双致密星引力波源的形成
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摘要
迄今为止,aLIGO/Virgo共探测到5次恒星级双黑洞并合和1次双中子星并合发出的引力波信号,宣布了引力波时代的全面到来.双白矮星的绕转和并合产生的引力波信号则是未来空间引力波探测器的主要探测目标.双星演化是这些双致密星形成的主要途径.本文从恒星演化出发,对这些双致密星引力波源的形成图像和面临的不确定性进行系统地介绍.这些不确定性主要来自大质量恒星星风、恒星后期演化、超新星爆发、双星演化的基本过程等.
The advanced LIGO/Virgo have detected gravitational-wave signals of merging double black holes and merging double neutron stars, opening a new window for astronomers to study the universe. The coming space gravitational wave detectors,such as Laser Interferometer Space Antenna(LISA) and Tian Qin, are expected to focus on gravitational-wave signals from double white dwarfs in close orbits and their mergers. Binary evolution is believed to be the major channel for the formation of those double compact objects. In this paper, we review the scenarios for the formation of various types of double compact objects and the uncertainties in the scenarios. The uncertainties are related to the stellar wind of massive stars, stellar evolution in late stages, supernova explosion/natal kicks, and the basic unsolved problems in binary evolution,etc.
The advanced LIGO/Virgo have detected gravitational-wave signals of merging double black holes and merging double neutron stars, opening a new window for astronomers to study the universe. The coming space gravitational wave detectors,such as Laser Interferometer Space Antenna(LISA) and Tian Qin, are expected to focus on gravitational-wave signals from double white dwarfs in close orbits and their mergers. Binary evolution is believed to be the major channel for the formation of those double compact objects. In this paper, we review the scenarios for the formation of various types of double compact objects and the uncertainties in the scenarios. The uncertainties are related to the stellar wind of massive stars, stellar evolution in late stages, supernova explosion/natal kicks, and the basic unsolved problems in binary evolution,etc.
引文
[1] Clark J P A,Eardley D M.Evolution of close neutron star binaries.Astrophys J,1977,215:311-322
2 Clark J P A,van den Heuvel E P J,Sutantyo W.Formation of neutron star binaries and their importance for gravitational radiation.Astron Astrophys,1979,72:120-128
3 Riles K.Gravitational waves:Sources,detectors and searches.Prog Particle Nucl Phys,2013,68:1-54
4 Lück H,Grote H,GEO 600.In:Ju L,ed.Advanced Gravitational Wave Detector.Cambridge:Cambridge University Press,2012.155-168
5 Somiya K.Detector configuration of KAGRA-the Japanese cryogenic gravitational-wave detector.Class Quantum Grav,2012,29:124007
6 Weisberg J M,Taylor J H.Binary Radio Pulsars.San Francisco:Astronomical Society of the Pacific,2005
7 Abbott B P,Abbott R,Abbott T D,et al.Observation of gravitational waves from a binary black hole merger.Phys Rev Lett,2016,116:061102
8 Abbott B P,Abbott R,Abbott T D,et al.GW151226:Observation of gravitational waves from a 22-solar-mass binary black hole coalescence.Phys Rev Lett,2016,116:241103
9 Abbott B P,Abbott R,Abbott T D,et al.GW170104:Observation of a 50-solar-mass binary black hole coalescence at redshift 0.2.Phys Rev Lett,2017,118:221101
10 Abbott B P,Abbott R,Abbott T D,et al.GW170814:A three-detector observation of gravitational waves from a binary black hole coalescence.Phys Rev Lett,2017,119:141101
11 Abbott B P,Abbott R,Abbott T D,et al.GW170608:Observation of a 19 solar-mass binary black hole coalescence.Astrophys J,2017,851:L35
12 Abbott B P,Abbott R,Abbott T D,et al.Gravitational waves and gamma-rays from a binary neutron star merger:GW170817 and GRB 170817A.Astrophys J,2017,848:L13
13 Abbott B P,Abbott R,Abbott T D,et al.Multi-messenger observations of a binary neutron star merger.Astrophys J,2017,848:L12
14 Marsh T R.Double white dwarfs and LISA.Class Quantum Grav,2011,28:094019
15 Luo J,Chen L S,Duan H Z,et al.Tian Qin:A space-borne gravitational wave detector.Class Quantum Grav,2016,33:035010
16 Wang B,Han Z.Progenitors of type Ia supernovae.New Astron Rev,2012,56:122-141
17 Riess A G,Filippenko A V,Challis P,et al.Observational evidence from supernovae for an accelerating universe and a cosmological constant.Astron J,1998,116:1009-1038
18 Perlmutter S,Aldering G,Goldhaber G,et al.Measurements of?andΛfrom 42 high-redshift supernovae.Astrophys J,1999,517:565-586
19 Timmes F X,Woosley S E,Weaver T A.Galactic chemical evolution:Hydrogen through zinc.Astrophys J Suppl Ser,1995,98:617-658
20 Langer N.Presupernova evolution of massive single and binary stars.Annu Rev Astron Astrophys,2012,50:107-164
21 Poelarends A J T,Herwig F,Langer N,et al.The supernova channel of super-AGB stars.Astrophys J,2008,675:614-625
22 Sana H.The multiplicity of massive stars:A 2016 view.Proc IAU,2016,12:110-117
23 Yoon S C,Langer N.Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts.Astron Astrophys,2005,443:643-648
24 Marchant P,Langer N,Podsiadlowski P,et al.A new route towards merging massive black holes.Astron Astrophys,2016,588:A50
25 Wellstein S,Langer N,Braun H.Formation of contact in massive close binaries.Astron Astrophys,2001,369:939-959
26 Burrows A,Hubbard W B,Saumon D,et al.An expanded set of brown dwarf and very low mass star models.Astrophys J,1993,406:158-171
27 Close L M,Thatte N,Nielsen E L,et al.New photometry and spectra of AB doradus C:An accurate mass determination of a young low-mass object with theoretical evolutionary tracks.Astrophys J,2007,665:736-743
28 Schnurr O,Casoli J,Chené A N,et al.The very massive binary NGC 3603-A1.Mon Not R Astron Soc-Lett,2008,389:L38-L42
29 Crowther P A,Schnurr O,Hirschi R,et al.The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted150Msolarstellar mass limit.Mon Not R Astron Soc,2010,408:731-751
30 Vink J S,Heger A,Krumholz M R,et al.Very massive stars in the local universe.Proc IAU,2012,10:51-79
31 Belkus H,Van Bever J,Vanbeveren D.The evolution of very massive stars.Astrophys J,2007,659:1576-1581
32 Yungelson L R,van den Heuvel E P J,Vink J S,et al.On the evolution and fate of super-massive stars.Astron Astrophys,2008,477:223-237
33 Shiode J H,Quataert E,Arras P.The stability of massive main-sequence stars as a function of metallicity.Mon Not R Astron Soc,2012,423:3397-3404
34 Abel T.The formation of the first star in the Universe.Science,2002,295:93-98
35 Susa H.The mass of the first stars.Astrophys J,2013,773:185
36 Salpeter E E.The luminosity function and stellar evolution.Astrophys J,1995,121:161-167
37 Weidner C,Pamm-Altenburg J,Kroupa P.The Galaxy-wide IMF-from Star Clusters to Galaxies.In:Treyer M,Wyder T,Neill J,Seibert M and Lee J,eds.UP2010:Have Observations Revealed A Variable Upper End of the Initial Mass Function?ASP Conference Series.San Francisco:Astronomical Society of the Pacic,2011.440:19
38 Lamb J B,Oey M S,Graus A S,et al.The initial mass function of field OB stars in the small magellanic cloud.Astrophys J,2013,763:101
39 Chomiuk L,Povich M S.Toward a unification of star formation rate determinations in the milky way and other galaxies.Astron J,2011,142:197
40 Kennicutt Jr R C,Evans Ii N J.Star formation in the milky way and nearby galaxies.Annu Rev Astron Astrophys,2012,50:531-608
41 Noriega-Crespo A.Star Formation in the Milky Way:The Infrared View.In:Torres D F,Reimer O,eds.Cosmic Rays in Star-Forming Environments.Advances in Solid State Physics Proceedings.Berlin-Heidelberg:Springer-Verlag,2013.34:29
42 Lau H H B,Gil-Pons P,Doherty C,et al.The end of super AGB and massive AGB stars.I.The instabilities that determine the final mass of AGB stars.Astron Astrophys,2012,542:A1
43 Han Z,Podsiadlowski P,Eggleton P P.A possible criterion for envelope ejection in asymptotic giant branch or first giant branch stars.Mon Not R Astron Soc,1994,270:121-130
44 Li Y.Introduction to Stellar Structure and Evolution(in Chinese).Beijing:Peking University Press,2014[李焱.恒星结构演化引论.北京:北京大学出版社,2014]
45 Podsiadlowski P,Langer N,Poelarends A J T,et al.The effects of binary evolution on the dynamics of core collapse and neutron star kicks.Astrophys J,2004,612:1044-1051
46 El Eid M F,Langer N.The evolution of very luminous stars.II.Pair creation supernova in massive Wolf-Rayet stars.Astron Astrophys,1986,167:274-281
47 Heger A,Woosley S E.The nucleosynthetic signature of population III.Astrophys J,2002,567:532-543
48 Waldman R.The most massive core-collapse supernova progenitors.Astrophys J,2008,685:1103-1108
49 Woosley S E,Blinnikov S,Heger A.Pulsational pair instability as an explanation for the most luminous supernovae.Nature,2007,450:390-392
50 Kitaura F S,Janka H T,Hillebrandt W.Explosions of O-Ne-Mg cores,the Crab supernova,and subluminous type II-P supernovae.Astron Astrophys,2006,450:345-350
51 Kasliwal M M,Kulkarni S R,Arcavi I,et al.PTF 10fqs:A luminous red nova in the spiral galaxy messier 99.Astrophys J,2011,730:134-144
52 Stephenson F R,Green D A.Historical Supernovae and their Remnants,International Series on Astronomy and Astrophysics.Oxford:Clarendon Press,2002
53 Tominaga N,Blinnikov S I,Nomoto K.Supernova explosions of super-asymptotic giant branch stars:Multicolor light curves of electron-capture supernovae.Astrophys J,2013,771:L12
54 van Veelen B.Supernovae Interacting with Their Circumstellar Media.Dissertation for Dcotoral Degree.Utrecht:Utrecht University,2010
55 Schlegel E M,Petre R.A chandra ACIS observation of the X-ray-luminous SN 1988Z.Astrophys J,2006,646:378-384
56 Ibeling D,Heger A.The metallicity dependence of the minimum mass for core-collapse supernovae.Astrophys J,2013,765:L43
57 Jones S,Hirschi R,Nomoto K,et al.Advanced burning stages and fate of 8-10 M⊙stars.Astrophys J,2013,772:150
58 Takahashi K,Yoshida T,Umeda H.Evolution of progenitors for electron capture supernovae.Astrophys J,2013,771:28
59 Poelarends A J T.Stellar Evolution at the Borderline of White Dwarf and Neutron Star Formation.Dissertation for Dcotoral Degree.Utrecht:Utrecht University,2007
60 Langer N,Norman C A,de Koter A,et al.Pair creation supernovae at low and high redshift.Astron Astrophys,2007,475:L19-L23
61 Gal-Yam A,Mazzali P,Ofek E O,et al.Supernova 2007bi as a pair-instability explosion.Nature,2009,462:624-627
62 Ofek E O,Cameron P B,Kasliwal M M,et al.SN 2006gy:An extremely luminous supernova in the galaxy NGC 1260.Astrophys J,2007,659:L13-L16
63 Smith N,Li W,Foley R J,et al.SN 2006gy:Discovery of the most luminous supernova ever recorded,powered by the death of an extremely massive star likeηcarinae.Astrophys J,2007,666:1116-1128
64 Smith N,Chornock R,Silverman J M,et al.Spectral evolution of the extraordinary type iin supernova 2006gy.Astrophys J,2010,709:856-883
65 Quimby R M,Kulkarni S R,Kasliwal M M,et al.Hydrogen-poor superluminous stellar explosions.Nature,2011,474:487-489
66 Arcavi I,Howell D A,Kasen D,et al.Energetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star.Nature,2017,551:210-213
67 Gunn J E,Ostriker J P.On the nature of pulsars.III.Analysis of observations.Astrophys J,1970,160:979
68 Shklovskii I S.Possible causes of the secular increase in pulsar periods.Sov Astron,1970,13:562-565
69 Lyne A G,Lorimer D R.High birth velocities of radio pulsars.Nature,1994,369:127-129
70 Hobbs G,Lorimer D R,Lyne A G,et al.A statistical study of 233 pulsar proper motions.Mon Not R Astron Soc,2005,360:974-992
71 Nordhaus J,Brandt T D,Burrows A,et al.The hydrodynamic origin of neutron star kicks.Mon Not R Astron Soc,2012,423:1805-1812
72 Wongwathanarat A,Janka H T,Müller E.Three-dimensional neutrino-driven supernovae:Neutron star kicks,spins,and asymmetric ejection of nucleosynthesis products.Astron Astrophys,2013,552:A126
73 Kaspi V M,Bailes M,Manchester R N,et al.Evidence from a precessing pulsar orbit for a neutron-star birth kick.Nature,1996,381:584-586
74 Prokhorov M E,Postnov K A.Direct observation of the kick during the birth of a neutron star in the binary pulsar PSR B1259-63.Astron Lett,1997,23:439-444
75 Behroozi P S,Ramirez-Ruiz E,Fryer C L.Interpreting short gamma-ray burst progenitor kicks and time delays using the host galaxy-dark matter halo connection.Astrophys J,2014,792:123-131
76 Pfahl E,Rappaport S,Podsiadlowski P,et al.A new class of high-mass X-ray binaries:Implications for core collapse and neutron star recoil.Astrophys J,2002,574:364-376
77 Corongiu A,Kramer M,Stappers B W,et al.The binary pulsar PSR J1811-1736:Evidence of a low amplitude supernova kick.Astron Astrophys,2007,462:703-709
78 Dewi J D M,Pols O R.The late stages of evolution of helium star-neutron star binaries and the formation of double neutron star systems.Mon Not R Astron Soc,2003,344:629-643
79 Podsiadlowski P,Dewi J D M,Lesaffre P,et al.The double pulsar J0737-3039:Testing the neutron star equation of state.Mon Not R Astron Soc,2005,361:1243-1249
80 Ferdman R D,Stairs I H,Kramer M,et al.The double pulsar:Evidence for neutron star formation without an iron core-collapse supernova.Astrophys J,2013,767:85
81 Guillemot L,Kramer M,Johnson T J,et al.Fermi LAT pulsed detection of PSR J0737-3039A in the double pulsar system.Astrophys J,2013,768:169
82 Burrows A,Hayes J.Pulsar recoil and gravitational radiation due to asymmetrical stellar collapse and explosion.Phys Rev Lett,1996,76:352-355
83 Jonker P G,Nelemans G.The distances to galactic low-mass X-ray binaries:Consequences for black hole luminosities and kicks.Mon Not RAstron Soc,2004,354:355-366
84 Fragos T,Willems B,Ivanova N et al.Black hole formation in X-ray binaries:The case of XTE J1118+48.In:di Salvo T,Israel G L,Piersant L,et al,eds.The Multicolored Landscape of Compact Objects and Their Explosive Origins.American Institute of Physics Conference Proceedings.Toronto,2007.924:673-676
85 Willems B,Henninger M,Levin T,et al.Understanding compact object formation and natal kicks.I.Calculation methods and the case of GROJ1655-40.Astrophys J,2005,625:324-346
86 Kuulkers E,Kouveliotou C,Belloni T,et al.MAXI J1659-152:The shortest orbital period black-hole transient in outburst.Astron Astrophys,2013,552:A32
87 Mirabel I F.Formation of a black hole in the dark.Science,2003,300:1119-1120
88 Wong T W,Valsecchi F,Fragos T,et al.Understanding compact object formation and natal kicks.III.The case of cygnus X-1.Astrophys J,2012,747:111
89 Nelemans G,Tauris T M,van den Heuvel E P J.Constraints on mass ejection in black hole formation derived from black hole X-ray binaries.Astron Astrophys,1999,352:L87-L90
90 Miller-Jones J C A,Jonker P G,Dhawan V,et al.The first accurate parallax distance to a black hole.Astrophys J,2009,706:L230-L234
91 Repetto S,Davies M B,Sigurdsson S.Investigating stellar-mass black hole kicks.Mon Not R Astron Soc,2012,425:2799-2809
92 Lipunov V M,Postnov K A,Prokhorov M E.Formation and coalescence of relativistic binary stars:The effect of kick velocity.Mon Not RAstron Soc,1997,288:245-259
93 Mapelli M,Colpi M,Zampieri L.Low metallicity and ultra-luminous X-ray sources in the cartwheel galaxy.Mon Not R Astron Soc-Lett,2009,395:L71-L75
94 Mapelli M,Zampieri L,Ripamonti E,et al.Dynamics of stellar black holes in young star clusters with different metallicities.I.Implications for X-ray binaries.Mon Not R Astron Soc,2013,429:2298-2314
95 Belczynski K,Bulik T,Fryer C L,et al.On the maximum mass of stellar black holes.Astrophys J,2010,714:1217-1226
96 Fryer C L,Belczynski K,Wiktorowicz G,et al.Compact remnant mass function:dependence on the explosion mechanism and metallicity.Astrophys J,2012,749:91
97 Maeder A.Stellar yields as a function of initial metallicity and mass limit for black hole formation.Astron Astrophys,1992,264:105-120
98 Vink J S,de Koter A,Lamers H J G L M.Mass-loss predictions for O and B stars as a function of metallicity.Astron Astrophys,2001,369:574-588
99 Vink J S,Muijres L E,Anthonisse B,et al.Wind modelling of very massive stars up to 300 solar masses.Astron Astrophys,2011,531:A132
100 Muijres L,Vink J S,de Koter A,et al.Mass-loss predictions for evolved very metal-poor massive stars.Astron Astrophys,2012,546:A42
101 Muijres L E,Vink J S,de Koter A,et al.Predictions for mass-loss rates and terminal wind velocities of massive O-type stars.Astron Astrophys,2012,537:A37
102 Meynet G,Maeder A.Stellar evolution with rotation.XI.Wolf-Rayet star populations at different metallicities.Astron Astrophys,2005,429:581-598
103 Vink J S,de Koter A.On the metallicity dependence of Wolf-Rayet winds.Astron Astrophys,2005,442:587-596
104 Grafener G,Hamann W R.Mass loss from late-type WN stars and its Z-dependence.Very massive stars approaching the Eddington limit.Astron Astrophys,2008,482:945-960
105 Tang J,Bressan A,Rosenfield P,et al.New PARSEC evolutionary tracks of massive stars at low metallicity:Testing canonical stellar evolution in nearby star-forming dwarf galaxies.Mon Not R Astron Soc,2014,445:4287-4305
106 Chen Y,Bressan A,Girardi L,et al.PARSEC evolutionary tracks of massive stars up to 350 M⊙at metallicities 0.0001≤Z≤0.04.Mon Not RAstron Soc,2015,452:1068-1080
107 Muijres L E,de Koter A,Vink J S,et al.Predictions of the effect of clumping on the wind properties of O-type stars.Astron Astrophys,2011,526:A32
108 Vink J S,Grafener G.The transition mass-loss rate:calibrating the role of line-driven winds in massive star evolution.Astrophys J,2012,751:L34
109 Grafener G,Vink J S,de Koter A,et al.The Eddington factor as the key to understand the winds of the most massive stars.Astron Astrophys,2011,535:A56
110 Vink J S.Mass loss and stellar superwinds.Phil Trans R Soc A,2017,375:20160269
111 Bestenlehner J M,Grafener G,Vink J S,et al.The VLT-FLAMES tarantula survey.XVII.Physical and wind properties of massive stars at the top of the main sequence.Astron Astrophys,2014,570:A38
112 Spera M,Mapelli M,Bressan A.The mass spectrum of compact remnants from the PARSEC stellar evolution tracks.Mon Not R Astron Soc,2015,451:4086-4103
113 Spera M,Mapelli M.Very massive stars,pair-instability supernovae and intermediate-mass black holes with the sevn code.Mon Not R Astron Soc,2017,470:4739-4749
114 Giacobbo N,Mapelli M,Spera M.Merging black hole binaries:The effects of progenitor’s metallicity,mass-loss rate and Eddington factor.Mon Not R Astron Soc,2018,474:2959-2974
115 Heger A,Fryer C L,Woosley S E,et al.How massive single stars end their life.Astrophys J,2003,591:288-300
116 Sana H,de Mink S E,de Koter A,et al.Binary interaction dominates the evolution of massive stars.Science,2012,337:444-446
117 Duch?ene G,Kraus A.Stellar multiplicity.Annu Rev Astron Astrophys,2013,51:269-310
118 Reggiani M,Meyer M R.Universality of the companion mass-ratio distribution.Astron Astrophys,2013,553:A124
119 Popova E I,Tutukov A V,Yungelson L R.Study of physical properties of spectroscopic binary stars.Astrophys Space Sci,1982,88:55-80
120 Kouwenhoven M B N,The Primordial Binary Population in the Association Sco OB2.Dissertation for Dcotoral Degree.Amsterdam:University of Amsterdam,2006
121 Kopal Z.Close Binary Systems.The International Astrophysics Series 5.London,New York:Chapman&Hall;Wiley,1959
122 Eggleton P P.Approximations to the radii of Roche lobes.Astrophys J,1983,268:368-369
123 Paczynski B.Gravitational waves and the evolution of close binaries.Acta Astron,1967,17:287-296
124 Hjellming M S,Webbnik R F.Thresholds for rapid mass transfer in binary systems.I.Polytropic models.Astrophys J,1987,318:794-808
125 Hjellming M.Rapid Mass Transfer in Binary Systems.Dissertation for Dcotoral Degree.Urbana-Champaign:University of Illinois at UrbanaChampaign,1989
126 Ge H,Hjellming M S,Webbink R F,et al.Adiabatic mass loss in binary stars.I.Computational method.Astrophys J,2010,717:724-738
127 Ge H,Webbink R F,Chen X,et al.Adiabatic mass loss in binary stars.II.From zero-age main sequence to the base of the giant branch.Astrophys J,2015,812:40
128 Paczynski B,Ziolkowski J,Zytkow A.On the Time-Scale of the Mass Transfer in Close Binaries.In:Hack M,ed.Mass Loss from Stars,Astrophysics and Space Science Library.Berlin Heidelberg:Springer-Verlag,1969.13:237
129 Paczynski B,Sienkiewicz R.Evolution of close binaries VIII.Mass exchange on the dynamical time scale.Acta Astron,1972,22:73-91
130 Soberman G E,Phinney E S,van den Heuvel E P J.Stability criteria for mass transfer in binary stellar evolution.Astron Astrophys,1997,327:620-635
131 Tauris T M,Savonije G J.Formation of millisecond pulsars.I.Evolution of low-mass X-ray binaries with Porb>2 days.Astron Astrophys,1999,350:928-944
132 Podsiadlowski P,Rappaport S,Pfahl E D.Evolutionary sequences for low-and intermediate-mass X-ray binaries.Astrophys J,2002,565:1107-1133
133 Pavlovskii K,Ivanova N.Mass transfer from giant donors.Mon Not R Astron Soc,2015,449:4415-4427
134 Lommen D,Yungelson L,van den Heuvel E,et al.Cygnus X-3 and the problem of the missing Wolf-Rayet X-ray binaries.Astron Astrophys,2005,443:231-241
135 Ghosh K K,Rappaport S,Tennant A F,et al.Discovery of a 3.6 hr eclipsing luminous X-ray binary in the galaxy NGC 4214.Astrophys J,2006,650:872-878
136 Podsiadlowski P,Joss P C,Hsu J J L.Presupernova evolution in massive interacting binaries.Astrophys J,1992,391:246-264
137 Paczynski B.Common envelope binaries.In:Proceedings of Structure and Evolution of Close Binary Systems(IAU Symposium 73)Conference in Cambridge.Cambridge,1975.75-80
138 Yungelson L R.Evolution of the secondary component of a close binary system.Nauchnye Informatsii,1973,27:93
139 Refsdal S,Roth M L,Weigert A.On the binary system AS Eri.Astron Astrophys,1974,36:113-122
140 Webbink R F.The evolution of low-mass close binary systems.IV.0.80M⊙+0.40M⊙catastrophic mass loss.Astrophys J,1977,211:881-889
141 Prialnik D,Livio M.The outcome of accretion on to a fully convective star expansion or contraction?Mon Not R Astron Soc,1985,216:37-52
142 Han Z,Webbink R F.Stability and energetics of mass transfer in double white dwarfs.Astron Astrophys,1999,349:L17-L20
143 Sparks W M,Stecher T P.Supernova:The result of the death spiral of a white dwarf into a red giant.Astrophys J,1974,188:149-153
144 Alexander M E,Chau W Y,Henriksen R N.Orbital evolution of a singly condensed,close binary,by mass loss from the primary and by accretion drag on the condensed member.Astrophys J,1976,204:879-888
145 Ivanova N,Justham S,Chen X,et al.Common envelope evolution:Where we stand and how we can move forward.Astron Astrophys Rev,2013,21:59-131
146 Drake J J,Sarna M J.X-ray evidence of the common envelope phase of V471 tauri.Astrophys J,2003,594:L55-L58
147 Sion E M,Bond H E,Lindler D,et al.Hubble space telescope FUV spectra of the post-common-envelope hyades binary V471 tauri.Astrophys J,2012,751:66
148 Kasliwal M M.Systematically bridging the gap between novae and supernovae.Publ Astron Soc Aust,2012,29:482-488
149 Ivanova N,Justham S,Nandez J L A,et al.Identification of the long-sought common-envelope events.Science,2013,339:433-435
150 Tylenda R,Kaminski T,Udalski A,et al.OGLE-2002-BLG-360:From a gravitational microlensing candidate to an overlooked red transient.Astron Astrophys,2013,555:A16
151 Mac Leod M,Ramirez-Ruiz E.On the accretion-fed growth of neutron stars during common envelope.Astrophys J,2015,798:L19
152 Mac Leod M,Ramirez-Ruiz E.Asymmetric accretion flows within a common envelope.Astrophys J,2015,803:41
153 Mac Leod M,Macias P,Ramirez-Ruiz E,et al.Lessons from the onset of a common envelope episode:The remarkable M31 2015 luminous red nova outburst.Astrophys J,2017,835:282
154 Mac Leod M,Antoni A,Murguia-Berthier A,et al.Common envelope wind tunnel:coefficients of drag and accretion in a simplified context for studying flows around objects embedded within stellar envelopes.Astrophys J,2017,838:56
155 Nandez J L A,Ivanova N,Lombardi Jr J C.Recombination energy in double white dwarf formation.Mon Not R Astron Soc-Lett,2015,450:L39-L43
156 Nandez J L A,Ivanova N.Common envelope events with low-mass giants:Understanding the energy budget.Mon Not R Astron Soc,2016,460:3992-4002
157 Ivanova N,Nandez J L A.Common envelope events with low-mass giants:understanding the transition to the slow spiral-in.Mon Not R Astron Soc,2016,462:362-381
158 Ohlmann S T,Ropke F K,Pakmor R,et al.Hydrodynamic moving-mesh simulations of the common envelope phase in binary stellar systems.Astrophys J,2016,816:L9
159 Ohlmann S T,Roepke F K,Pakmor R,et al.Magnetic field amplification during the common envelope phase.Mon Not R Astron Soc-Lett,2016,462:L121-L125
160 Ohlmann S T,Roepke F K,Pakmor R,et al.Constructing stable 3D hydrodynamical models of giant stars.Astron Astrophys,2017,599:A5
161 Van Den Heuvel E P J.Late stages of close binary systems.Symp-Int Astron Union,1976,73:35-61
162 Tutukov A V,Yungelson L R.Evolution of massive common envelope binaries and mass loss.In:Proceedings of Mass Loss and Evolution of O-type Stars,IAU Symposium 83 in Vancouver Island.Canada,1978.401
163 Webbink R F.Double white dwarfs as progenitors of R Coronae Borealis stars and Type I supernovae.Astrophys J,1984,277:355-360
164 Kashi A,Soker N.A circumbinary disc in the final stages of common envelope and the core-degenerate scenario for Type Ia supernovae.Mon Not R Astron Soc,2011,417:1466-1479
165 Ivanova N,Chaichenets S.Common envelope:Enthalpy consideration.Astrophys J,2011,731:L36-39
166 Ivanova N.Common envelope:On the mass and the fate of the remnant.Astrophys J,2011,730:76
167 Xu X J,Li X D.On the binding energy parameterλof common envelope evolution.Astrophys J,2010,716:114-121
168 De Marco O,Passy J C,Moe M,et al.On theαformalism for the common envelope interaction.Mon Not R Astron Soc,2011,411:2277-2292
169 Davis P J,Kolb U,Knigge C.Is the common envelope ejection efficiency a function of the binary parameters?Mon Not R Astron Soc,2012,419:287-303
170 Zorotovic M,Schreiber M R,Gansicke B T,et al.Post-common-envelope binaries from SDSS.IX:Constraining the common-envelope efficiency.Astron Astrophys,2010,520:A86
171 Davis P J,Kolb U,Willems B.A comprehensive population synthesis study of post-common envelope binaries.Mon Not R Astron Soc,2010,403:179-195
172 Toonen S,Nelemans G.The effect of common-envelope evolution on the visible population of post-common-envelope binaries.Astron Astrophys,2013,557:A87
173 Zorotovic M,Schreiber M R,Garc?a-Berro E,et al.Monte Carlo simulations of post-common-envelope white dwarf+main sequence binaries:The effects of including recombination energy.Astron Astrophys,2014,568:A68
174 Camacho J,Torres S,Garc?a-Berro E,et al.Monte Carlo simulations of post-common-envelope white dwarf+main sequence binaries:Comparison with the SDSS DR7 observed sample.Astron Astrophys,2014,566:A86
175 Nelemans G,Yungelson L R,Portegies Zwart S F,et al.Population synthesis for double white dwarfs.I.Close detached systems.Astron Astrophys,2001,365:491-507
176 Nelemans G,Verbunt F,Yungelson L R,et al.Reconstructing the evolution of double helium white dwarfs:Envelope loss without spiral-in.Astron Astrophys,2000,360:1011-1018
177 Nelemans G,Tout C A.Reconstructing the evolution of white dwarf binaries:Further evidence for an alternative algorithm for the outcome of the common-envelope phase in close binaries.Mon Not R Astron Soc,2005,356:753-764
178 van der Sluys M V,Verbunt F,Pols O R.Modelling the formation of double white dwarfs.Astron Astrophys,2006,460:209-228
179 Gosnell N M,Mathieu R D,Geller A M,et al.Detection of white dwarf companions to blue stragglers in the open cluster NGC 188:Direct evidence for recent mass transfer.Astrophys J,2014,783:L8
180 Gosnell N M,Mathieu R D,Geller A M,et al.Implications for the formation of blue straggler stars from HST ultraviolet observations of NGC188.Astrophys J,2015,814:163
181 Postnov K A,Yungelson L R.The evolution of compact binary star systems.Living Rev Relativ,2014,17:3
182 Flannery B P,van den Heuvel E P J.On the origin of the binary pulsar PSR 1913+16.Astrophys J,1975,39:61-67
183 de Loore C,de Gréve J P,de Cuyper J P.Evolution of massive close binaries.II.The POST X-ray binary stage:Origin of run-away and binary pulsars.Astrophys Space Sci,1975,36:219-225
184 Srinivasan G,van den Heuvel E P J.Some constraints on the evolutionary history of the binary pulsar PSR 1913+16.Astron Astrophys,1982,108:143-147
185 Backer D C,Kulkarni S R,Heiles C,et al.A millisecond pulsar.Nature,1982,300:615-618
186 van den Heuvel E P J.Formation of double neutron stars,millisecond pulsars and double black holes.J Astrophys Astron,2017,38:45.Ar Xiv:1709.07636
187 Tauris T M,Kramer M,Freire P C C,et al.Formation of double neutron star systems.Astrophys J,2017,846:170
188 Nugis T,Lamers H J G L M.Mass-loss rates of Wolf-Rayet stars as a function of stellar parameters.Astron Astrophys,2000,360:227-244
189 Fadeyev Y A,Novikova M F.Radial pulsations of helium stars with masses from 1 to 10 M⊙.Astron Lett,2003,29:522-529
190 Fadeyev Y A,Novikova M F.Radial pulsations of helium stars with masses from 10 to 50M⊙.Astron Lett,2004,30:707-714
191 Miroshnichenko A S.Toward understanding the B[e]phenomenon.I.Definition of the galactic FS CMa stars.Astrophys J,2007,667:497-504
192 Miroshnichenko A S,The B[e]phenomenon:Forty years of studies.Astron Soc Pacific Conf Ser,2017,508:285
193 Khokhlov S A,Miroshnichenko A S,Zharikov S V,et al.Toward understanding the B[e]phenomenon.VII.AS 386,a single-lined binary with a candidate black hole component.Astrophys J,2018,in press.Ar Xiv:1803.03892
194 De Donder E,Vanbeveren D,van Bever J.The number of O-type runaways,the number of O and Wolf-Rayet stars with a compact companion and the formation rate of double pulsars predicted by massive close binary evolution.Astron Astrophys,1997,318:812-818
195 Portegies Zwart S F,Yungelson L R.Formation and evolution of binary neutron stars.Astron Astrophys,1998,332:173-188
196 Kuranov A G,Popov S B,Postnov K A.Pulsar spin-velocity alignment from single and binary neutron star progenitors.Mon Not R Astron Soc,2009,395:2087-2094
197 Ergma E,Yungelson L R,CYG X-3:Can the compact object be a black hole?Astron Astrophys,1998,333:151-158
198 Linden T,Valsecchi F,Kalogera V.On the rarity of X-ray binaries with naked helium donors.Astrophys J,2012,748:114
199 Thorne K S,Zytkow A N.Red giants and supergiants with degenerate neutron cores.Astrophys J,1975,199:L19-L24
200 Barkov M V,Bisnovatyi-Kogan G S,Lamzin S A.The thermal evolution of thorne-zytkow objects.Astron Rep,2001,45:230-235
201 Tout C A,Zytkow A N,Church R P,et al.HV2112,a Thorne-Zytkow object or a super asymptotic giant branch star.Mon Not R Astron Soc-Lett,2014,445:L36-L40
202 Foellmi C,Moffat A F J.Are peculiar wolf-rayet stars of type WN8 Thorne-Zytkow Objects?Astron Soc Pacific Conf Ser,2002,263:123
203 Colgate S A.Neutron-star formation,thermonuclear supernovae,and heavy-element reimplosion.Astrophys J,1971,163:221-230
204 Chevalier R A.Neutron star accretion in a stellar envelope.Astrophys J,1993,411:L33-L36
205 Botticella M T,Smartt S J,Kennicutt Jr R C,et al.A comparison between star formation rate diagnostics and rate of core collapse supernovae within 11 Mpc.Astron Astrophys,2012,537:A132
206 van den Heuvel E P J.X-ray binaries and their descendants:Binary radio pulsars;evidence for three classes of neutron stars?In:Proceedings of5th Integral Workshop On The Integral Universe.ESA Special Publication,2004,552.185
207 Schwab J,Podsiadlowski P,Rappaport S.Further evidence for the bimodal distribution of neutron-star masses.Astrophys J,2010,719:722-727
208 Knigge C,Coe M J,Podsiadlowski P.Two populations of X-ray pulsars produced by two types of supernova.Nature,2011,479:372-375
209 van den Heuvel E P J.Compact stars and the evolution of binary systems.Bull Astrono Soc India,2011,39:1-20
210 Iben I J,Tutukov A V,Yungelson L R.A model of the galactic X-ray binary population.II.Low-mass X-ray binaries in the galactic disk.Astrophys J Suppl Ser,1995,100:233
211 Kalogera V,Webbink R F.Formation of low-mass X-ray binaries.I.Constraints on hydrogen-rich donors at the onset of the X-ray phase.Astrophys J,1996,458:301
212 Kalogera V,Webbink R F.Formation of low-mass X-ray binaries.II.Common envelope evolution of primordial binaries with extreme mass ratios.Astrophys J,1998,493:351-367
213 Tutukov A V,Fedorova A V.Evolution of close stellar binaries with black holes under the action of gravitational radiation and magnetic and induced stellar winds of the donor.Astron Rep,2002,46:765-778
214 Wang B,Podsiadlowski P,Han Z.He-accreting carbon-oxygen white dwarfs and type Ia supernovae.Mon Not R Astron Soc,2017,472:1593-1599
215 Ziosi B M,Mapelli M,Branchesi M,et al.Dynamics of stellar black holes in young star clusters with different metallicities.II.Black hole-black hole binaries.Mon Not R Astron Soc,2014,441:3703-3717
216 Fryer C L.Mass limits for black hole formation.Astrophys J,1999,522:413-418
217 van den Heuvel E P J,Habets G M H J.Observational lower mass limit for black hole formation derived from massive X-ray binaries.Nature,1984,309:598-600
218 Woosley S E,Langer N,Weaver T A.The presupernova evolution and explosion of helium stars that experience mass loss.Astrophys J,1995,448:315-338
219 Portegies Z S F,Verbunt F,Ergma E.The formation of black-holes in low-mass X-ray binaries.Astron Astrophys,1997,321:207-212
220 Ergma E,van den Heuvel E P J.On the initial progenitor masses of stellar mass black holes and neutron stars.Astron Astrophys,1998,331:L29-L32
221 Brown G E,Heger A,Langer N,et al.Formation of high mass X-ray black hole binaries.New Astron,2001,6:457-470
222 Kochanek C S.Failed supernovae explain the compact remnant mass function.Astrophys J,2014,785:28
223 Muno M P,Clark J S,Crowther P A,et al.A neutron star with a massive progenitor in westerlund 1.Astrophys J,2006,636:L41-L44
224 Timmes F X,Woosley S E,Weaver T A.The neutron star and black hole initial mass function.Astrophys J,1996,457:834-843
225 Remillard R A,Mc Clintock J E.X-ray properties of black-hole binaries.Annu Rev Astron Astrophys,2006,44:49-92
226 Fryer C L,Kalogera V.Theoretical black hole mass distributions.Astrophys J,2001,554:548-560
227 Georgy C,Meynet G,Walder R,et al.The different progenitors of type Ib,Ic SNe,and of GRB.Astron Astrophys,2009,502:611-622
228 Linden T,Kalogera V,Sepinsky J F,et al.The effect of starburst metallicity on bright X-ray binary formation pathways.Astrophys J,2010,725:1984-1994
229 Belczynski K,Holz D E,Bulik T,et al.The first gravitational-wave source from the isolated evolution of two stars in the 40-100 solar mass range.Nature,2016,534:512-515
230 Crowther P A,Barnard R,Carpano S,et al.NGC 300 X-1 is a Wolf-Rayet/black hole binary.Mon Not R Astron Soc-Lett,2010,403:L41-L45
231 Foucart F,Deaton M B,Duez M D,et al.Black-hole-neutron-star mergers at realistic mass ratios:Equation of state and spin orientation effects.Phys Rev D,2013,87:084006
232 Endal A S,Sofia S.The evolution of rotating stars.II.Calculations with time-dependent redistribution of angular momentum for 7-and 10-solarmass stars.Astrophys J,1978,220:279-290
233 Zahn J P.Circulation and turbulence in rotating stars.Astron Astrophys,1992,265:115-132
234 Maeder A.Evidences for a bifurcation in massive star evolution.The ON-blue stragglers.Astron Astrophys,1987,178:159-169
235 Woosley S E,Heger A.The progenitor stars of gamma-ray bursts.Astrophys J,2006,637:914-921
236 Brott I,de Mink S E,Cantiello M,et al.Rotating massive main-sequence stars.I.Grids of evolutionary models and isochrones.Astron Astrophys,2011,530:A115
237 Koehler K,Langer N,de Koter A,et al.The evolution of rotating very massive stars with LMC composition.Astron Astrophys,2015,573:A71
238 Szécsi D,Langer N,Yoon S C,et al.Low-metallicity massive single stars with rotation.Evolutionary models applicable to I Zwicky 18.Astron Astrophys,2015,581:A15
239 de Mink S E,Cantiello M,Langer N,et al.Rotational mixing in massive binaries.Detached short-period systems.Astron Astrophys,2009,497:243-253
240 Mandel I,de Mink S E.Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries.Mon Not R Astron Soc,2016,458:2634-2647
241 Song H F,Meynet G,Maeder A,et al.Massive star evolution in close binaries.Conditions for homogeneous chemical evolution.Astron Astrophys,2016,585:A120
242 Marchant P,Langer N,Podsiadlowski P,et al.Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity.Astron Astrophys,2017,604:A55
243 Kilic M,Brown W R,Kenyon S J,et al.The shortest period detached binary white dwarf system.Mon Not R Astron Soc-Lett,2011,413:L101-L105
244 Brown W R,Kilic M,Hermes J J,et al.A 12 minute orbital period detached white dwarf eclipsing binary.Astrophys J,2011,737:L23
245 Hermes J J,Kilic M,Brown W R,et al.Rapid orbital decay in the 12.75-minute binary white dwarf J0651+2844.Astrophys J,2012,757:L21
246 Nelemans G.Galactic Binaries with e LISA.In:Proceedings of the 9th LISA Symposium.Bibliotheque Nationale de France,Paris,2012.ASPConference Series,2013,467.27
247 Brown W R,Kilic M,Prieto C A,et al.The ELM Survey.I.A complete sample of extremely low-mass white dwarfs.Astrophys J,2010,723:1072-1081
248 Kilic M,Brown W R,Prieto C A,et al.The ELM survey.II.Twelve binary white dwarf merger systems.Astrophys J,2011,727:3
249 Brown W R,Kilic M,Allende Prieto C,et al.The ELM survey.III.A successful targeted survey for extremely low mass white dwarfs.Astrophys J,2012,744:142
250 Kilic M,Brown W R,Allende Prieto C,et al.The ELM survey.IV.24 white dwarf merger systems.Astrophys J,2012,751:141
251 Brown W R,Kilic M,Allende Prieto C,et al.The ELM survey.V.Merging massive white dwarf binaries.Astrophys J,2013,769:66
252 Gianninas A,Kilic M,Brown W R,et al.The ELM survey.VI.Eleven new double degenerates.Astrophys J,2015,812:167
253 Brown W R,Gianninas A,Kilic M,et al.The ELM survey.VII.Orbital properties of low-mass white dwarf binaries.Astrophys J,2016,818:155
254 Brown W R,Kilic M,Kenyon S J,et al.Most double degenerate low-mass white dwarf binaries merge.Astrophys J,2016,824:46
255 Kilic M,Hermes J J,Gianninas A,et al.Found:The progenitors of AM CVn and supernovae Ia.Mon Not R Astron Soc-Lett,2014,438:L26-L30
256 Han Z.The formation of double degenerates and related objects.Mon Not R Astron Soc,1998,296:1019-1040
257 Istrate A G,M Tauris T,Langer N.The formation of low-mass helium white dwarfs orbiting pulsars.Evolution of low-mass X-ray binaries below the bifurcation period.Astron Astrophys,2014,571:A45
258 Chen X,Maxted P F L,Li J,et al.The formation of EL CVn-type binaries.Mon Not R Astron Soc,2017,467:1874-1889
259 Han Z,Podsiadlowski P,Maxted P F L,et al.The origin of subdwarf B stars.I.The formation channels.Mon Not R Astron Soc,2002,336:449-466
260 Han Z,Podsiadlowski P,Maxted P F L,et al.The origin of subdwarf B stars.II.Mon Not R Astron Soc,2003,341:669-691
261 Zhang X,Jeffery C S.Evolutionary models for double helium white dwarf mergers and the formation of helium-rich hot subdwarfs.Mon Not RAstron Soc,2012,419:452-464
262 Maoz D,Hallakoun N,Badenes C.The separation distribution and merger rate of double white dwarfs:Improved constraints.Mon Not R Astron Soc,2018,in press.Ar Xiv:1801.04275
263 Solheim J E.AM CVn stars:Status and challenges.Publ Astron Soc Pac,2010,122:1133-1163
264 Pringle J E,Webbink R F.Ariel 1118-61-A very close binary system.Mon Not R Astron Soc,1975,172:493-500
265 Tutukov A V,Yungelson L R.On the influence of emission of gravitational waves on the evolution of low-mass close binary stars.Acta Astron,1979,29:665-680
266 Nelemans G,Yungelson L R,Portegies Zwart S F.The gravitational wave signal from the Galactic disk population of binaries containing two compact objects.Astron Astrophys,2001,375:890-898
267 Zapolsky H S,Salpeter E E.The mass-radius relation for cold spheres of low mass.Astrophys J,1969,158:809-813
268 Nauenberg M.Analytic approximations to the mass-radius relation and energy of zero-temperature stars.Astrophys J,1972,175:417
269 Verbunt F,Rappaport S.Mass transfer instabilities due to angular momentum flows in close binaries.Astrophys J,1988,332:193-198
270 Tutukov A V,Fedorova A V,Formation and evolution of close binaries containing helium donors.Sov Astron,1989,33:606-613
271 Tutukov A,Yungelson L.Double-degenerate semidetached binaries with helium secondaries:Cataclysmic variables,supersoft X-ray sources,supernovae and accretion-induced collapses.Mon Not R Astron Soc,1996,280:1035-1045
272 Nelemans G,Yungelson L R,Portegies Zwart S F.Short-period AM CVn systems as optical,X-ray and gravitational-wave sources.Mon Not RAstron Soc,2004,349:181-192
273 Ruiter A J,Belczynski K,Benacquista M,et al.The LISA gravitational wave foreground:A study of double white dwarfs.Astrophys J,2010,717:1006-1021
274 Deloye C J,Taam R E,Winisdoerffer C,et al.The thermal evolution of the donors in AM canum venaticorum binaries.Mon Not R Astron Soc,2007,381:525-542
275 D’Antona F,Ventura P,Burderi L,et al.Modeling the closest double degenerate system RX J0806.3+1527 and its decreasing period.Astrophys J,2006,653:1429-1434
276 Kaplan D L,Bildsten L,Steinfadt J D R.Orbital evolution of compact white dwarf binaries.Astrophys J,2012,758:64
277 Holcomb C,Guillochon J,De Colle F,et al.Conditions for successful helium detonations in astrophysical environments.Astrophys J,2013,771:14
278 Paczynski B.Evolution of Single Stars.IV.Helium stars.Acta Astron,1971,21:1-14
279 Savonije G J,de Kool M,van den Heuvel E P J.The minimum orbital period for ultra-compact binaries with helium burning secondaries.Astron Astrophys,1986,155:51-57
280 Iben I J,Tutukov A V.Helium star cataclysmics.Astrophys J,1991,370:615-629
281 Ivanova N,Taam R E.Thermal timescale mass transfer and the evolution of white dwarf binaries.Astrophys J,2004,601:1058-1066
282 Yungelson L R.Evolution of low-mass helium stars in semidetached binaries.Astron Lett,2008,34:620-634
283 Fink M,Ropke F K,Hillebrandt W,et al.Double-detonation sub-Chandrasekhar supernovae:Can minimum helium shell masses detonate the core?Astron Astrophys,2010,514:A53
284 Sim S A,Fink M,Kromer M,et al.2D simulations of the double-detonation model for thermonuclear transients from low-mass carbon-oxygen white dwarfs.Mon Not R Astron Soc,2012,420:3003-3016
285 Moll R,Woosley S E.Multi-dimensional models for double detonation in sub-chandrasekhar mass white dwarfs.Astrophys J,2013,774:137
286 Roelofs G H A,Groot P J,Nelemans G,et al.On the orbital periods of the AM CVn stars HP Librae and V803 Centauri.Mon Not R Astron Soc,2007,379:176-182
287 Carter P J,Marsh T R,Steeghs D,et al.A search for the hidden population of AM CVn binaries in the sloan digital sky survey.Mon Not RAstron Soc,2013,429:2143-2160
288 Zhang X F,Liu J Z,Jeffery C S,et al.The double helium-white dwarf channel for the formation of AM CVn binaries.Res Astron Astrophys,2018,18:009
289 Belczynski K,Taam R E.Galactic populations of ultracompact binaries.Astrophys J,2004,603:690-696
290 Miller G E,Scalo J M.The initial mass function and stellar birthrate in the solar neighborhood.Astrophys J Suppl Ser,1979,41:513-547
291 Yungelson L R,Livio M,Tutukov A V,et al.Are the observed frequencies of double degenerates and SN IA contradictory?Astrophys J,1994,420:336-340
292 Nelemans G,Portegies Zwart S F,Verbunt F,et al.Population synthesis for double white dwarfs.II.Semi-detached systems:AM CVn stars.Astron Astrophys,2001,368:939-949
293 Toonen S,Claeys J S W,Mennekens N,et al.Pop CORN:Hunting down the differences between binary population synthesis codes.Astron Astrophys,2014,562:A14
294 Tutukov A V,Yungel Son L R.The merger rate of neutron star and black hole binaries.Mon Not R Astron Soc,1993,260:675-678
295 Lipunov V M,Postnov K A,Prokhorov M E.Black holes and gravitational waves:Possibilities for simultaneous detection using rst-generation laser interferometers.Astron Lett,1997,23:492-497
296 Voss R,Tauris T M.Galactic distribution of merging neutron stars and black holes-prospects for short gamma-ray burst progenitors and LIGO/VIRGO.Mon Not R Astron Soc,2003,342:1169-1184
297 O’Shaughnessy R,Kim C,Fragos T,et al.Constraining population synthesis models via the binary neutron star population.Astrophys J,2005,633:1076-1084
298 Dominik M,Belczynski K,Fryer C,et al.Double compact objects.I.The significance of the common envelope on merger rates.Astrophys J,2012,759:52
299 Mennekens N,Vanbeveren D.Massive double compact object mergers:Gravitational wave sources and r-process element production sites.Astron Astrophys,2014,564:A134
300 Belczynski K,Repetto S,Holz D E,et al.Compact binary merger rates:Comparison with LIGO/Virgo upper limits.Astrophys J,2016,819:108
301 Belczynski K,Heger A,Gladysz W,et al.The effect of pair-instability mass loss on black-hole mergers.Astron Astrophys,2016,594:A97
302 Belczynski K,Ryu T,Perna R,et al.On the likelihood of detecting gravitational waves from Population III compact object binaries.Mon Not RAstron Soc,2017,471:4702-4721
303 Eldridge J J,Stanway E R.BPASS predictions for binary black hole mergers.Mon Not R Astron Soc,2016,462:3302-3313
304 Pavlovskii K,Ivanova N,Belczynski K,et al.Stability of mass transfer from massive giants:Double black hole binary formation and ultraluminous X-ray sources.Mon Not R Astron Soc,2017,465:2092-2100
305 van den Heuvel E P J,Portegies Zwart S F,de Mink S E.Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer.Mon Not R Astron Soc,2017,471:4256-4264
306 Hainich R,Oskinova L M,Shenar T,et al.Observational properties of massive black hole binary progenitors.Astron Astrophys,2018,609:A94
307 Stevenson S,Vigna-Gomez A,Mandel I,et al.Formation of the first three gravitational-wave observations through isolated binary evolution.Nat Commun,2017,8:14906
308 Chruslinska M,Belczynski K,Klencki J,et al.Double neutron stars:Merger rates revisited.Mon Not R Astron Soc,2018,474:2937-2958
309 Vink J S,de Koter A.Predictions of variable mass loss for luminous blue variables.Astron Astrophys,2002,393:543-553
310 Fishbach M,Holz D E.Where are LIGO’s big black holes?Astrophys J,2017,851:L25
311 Kim C,Perera B B P,Mc Laughlin M A.Implications of PSR J0737-3039B for the Galactic NS-NS binary merger rate.Mon Not R Astron Soc,2015,448:928-938
312 Bray J C,Eldridge J J.Neutron star kicks and their relationship to supernovae ejecta mass.Mon Not R Astron Soc,2016,461:3747-3759
313 de Mink S E,Belczynski K.Merger rates of double neutron stars and stellar origin black holes:The impact of initial conditions on binary evolution predictions.Astrophys J,2015,814:58
314 Gupta A,Arun K G,Sathyaprakash B S.Implications of binary black hole detections on the merger rates of double neutron stars and neutron star-black holes.Astrophys J,2017,849:L14
315 de Mink S E,Mandel I.The chemically homogeneous evolutionary channel for binary black hole mergers:Rates and properties of gravitationalwave events detectable by advanced LIGO.Mon Not R Astron Soc,2016,460:3545-3553
2 Clark J P A,van den Heuvel E P J,Sutantyo W.Formation of neutron star binaries and their importance for gravitational radiation.Astron Astrophys,1979,72:120-128
3 Riles K.Gravitational waves:Sources,detectors and searches.Prog Particle Nucl Phys,2013,68:1-54
4 Lück H,Grote H,GEO 600.In:Ju L,ed.Advanced Gravitational Wave Detector.Cambridge:Cambridge University Press,2012.155-168
5 Somiya K.Detector configuration of KAGRA-the Japanese cryogenic gravitational-wave detector.Class Quantum Grav,2012,29:124007
6 Weisberg J M,Taylor J H.Binary Radio Pulsars.San Francisco:Astronomical Society of the Pacific,2005
7 Abbott B P,Abbott R,Abbott T D,et al.Observation of gravitational waves from a binary black hole merger.Phys Rev Lett,2016,116:061102
8 Abbott B P,Abbott R,Abbott T D,et al.GW151226:Observation of gravitational waves from a 22-solar-mass binary black hole coalescence.Phys Rev Lett,2016,116:241103
9 Abbott B P,Abbott R,Abbott T D,et al.GW170104:Observation of a 50-solar-mass binary black hole coalescence at redshift 0.2.Phys Rev Lett,2017,118:221101
10 Abbott B P,Abbott R,Abbott T D,et al.GW170814:A three-detector observation of gravitational waves from a binary black hole coalescence.Phys Rev Lett,2017,119:141101
11 Abbott B P,Abbott R,Abbott T D,et al.GW170608:Observation of a 19 solar-mass binary black hole coalescence.Astrophys J,2017,851:L35
12 Abbott B P,Abbott R,Abbott T D,et al.Gravitational waves and gamma-rays from a binary neutron star merger:GW170817 and GRB 170817A.Astrophys J,2017,848:L13
13 Abbott B P,Abbott R,Abbott T D,et al.Multi-messenger observations of a binary neutron star merger.Astrophys J,2017,848:L12
14 Marsh T R.Double white dwarfs and LISA.Class Quantum Grav,2011,28:094019
15 Luo J,Chen L S,Duan H Z,et al.Tian Qin:A space-borne gravitational wave detector.Class Quantum Grav,2016,33:035010
16 Wang B,Han Z.Progenitors of type Ia supernovae.New Astron Rev,2012,56:122-141
17 Riess A G,Filippenko A V,Challis P,et al.Observational evidence from supernovae for an accelerating universe and a cosmological constant.Astron J,1998,116:1009-1038
18 Perlmutter S,Aldering G,Goldhaber G,et al.Measurements of?andΛfrom 42 high-redshift supernovae.Astrophys J,1999,517:565-586
19 Timmes F X,Woosley S E,Weaver T A.Galactic chemical evolution:Hydrogen through zinc.Astrophys J Suppl Ser,1995,98:617-658
20 Langer N.Presupernova evolution of massive single and binary stars.Annu Rev Astron Astrophys,2012,50:107-164
21 Poelarends A J T,Herwig F,Langer N,et al.The supernova channel of super-AGB stars.Astrophys J,2008,675:614-625
22 Sana H.The multiplicity of massive stars:A 2016 view.Proc IAU,2016,12:110-117
23 Yoon S C,Langer N.Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts.Astron Astrophys,2005,443:643-648
24 Marchant P,Langer N,Podsiadlowski P,et al.A new route towards merging massive black holes.Astron Astrophys,2016,588:A50
25 Wellstein S,Langer N,Braun H.Formation of contact in massive close binaries.Astron Astrophys,2001,369:939-959
26 Burrows A,Hubbard W B,Saumon D,et al.An expanded set of brown dwarf and very low mass star models.Astrophys J,1993,406:158-171
27 Close L M,Thatte N,Nielsen E L,et al.New photometry and spectra of AB doradus C:An accurate mass determination of a young low-mass object with theoretical evolutionary tracks.Astrophys J,2007,665:736-743
28 Schnurr O,Casoli J,Chené A N,et al.The very massive binary NGC 3603-A1.Mon Not R Astron Soc-Lett,2008,389:L38-L42
29 Crowther P A,Schnurr O,Hirschi R,et al.The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted150Msolarstellar mass limit.Mon Not R Astron Soc,2010,408:731-751
30 Vink J S,Heger A,Krumholz M R,et al.Very massive stars in the local universe.Proc IAU,2012,10:51-79
31 Belkus H,Van Bever J,Vanbeveren D.The evolution of very massive stars.Astrophys J,2007,659:1576-1581
32 Yungelson L R,van den Heuvel E P J,Vink J S,et al.On the evolution and fate of super-massive stars.Astron Astrophys,2008,477:223-237
33 Shiode J H,Quataert E,Arras P.The stability of massive main-sequence stars as a function of metallicity.Mon Not R Astron Soc,2012,423:3397-3404
34 Abel T.The formation of the first star in the Universe.Science,2002,295:93-98
35 Susa H.The mass of the first stars.Astrophys J,2013,773:185
36 Salpeter E E.The luminosity function and stellar evolution.Astrophys J,1995,121:161-167
37 Weidner C,Pamm-Altenburg J,Kroupa P.The Galaxy-wide IMF-from Star Clusters to Galaxies.In:Treyer M,Wyder T,Neill J,Seibert M and Lee J,eds.UP2010:Have Observations Revealed A Variable Upper End of the Initial Mass Function?ASP Conference Series.San Francisco:Astronomical Society of the Pacic,2011.440:19
38 Lamb J B,Oey M S,Graus A S,et al.The initial mass function of field OB stars in the small magellanic cloud.Astrophys J,2013,763:101
39 Chomiuk L,Povich M S.Toward a unification of star formation rate determinations in the milky way and other galaxies.Astron J,2011,142:197
40 Kennicutt Jr R C,Evans Ii N J.Star formation in the milky way and nearby galaxies.Annu Rev Astron Astrophys,2012,50:531-608
41 Noriega-Crespo A.Star Formation in the Milky Way:The Infrared View.In:Torres D F,Reimer O,eds.Cosmic Rays in Star-Forming Environments.Advances in Solid State Physics Proceedings.Berlin-Heidelberg:Springer-Verlag,2013.34:29
42 Lau H H B,Gil-Pons P,Doherty C,et al.The end of super AGB and massive AGB stars.I.The instabilities that determine the final mass of AGB stars.Astron Astrophys,2012,542:A1
43 Han Z,Podsiadlowski P,Eggleton P P.A possible criterion for envelope ejection in asymptotic giant branch or first giant branch stars.Mon Not R Astron Soc,1994,270:121-130
44 Li Y.Introduction to Stellar Structure and Evolution(in Chinese).Beijing:Peking University Press,2014[李焱.恒星结构演化引论.北京:北京大学出版社,2014]
45 Podsiadlowski P,Langer N,Poelarends A J T,et al.The effects of binary evolution on the dynamics of core collapse and neutron star kicks.Astrophys J,2004,612:1044-1051
46 El Eid M F,Langer N.The evolution of very luminous stars.II.Pair creation supernova in massive Wolf-Rayet stars.Astron Astrophys,1986,167:274-281
47 Heger A,Woosley S E.The nucleosynthetic signature of population III.Astrophys J,2002,567:532-543
48 Waldman R.The most massive core-collapse supernova progenitors.Astrophys J,2008,685:1103-1108
49 Woosley S E,Blinnikov S,Heger A.Pulsational pair instability as an explanation for the most luminous supernovae.Nature,2007,450:390-392
50 Kitaura F S,Janka H T,Hillebrandt W.Explosions of O-Ne-Mg cores,the Crab supernova,and subluminous type II-P supernovae.Astron Astrophys,2006,450:345-350
51 Kasliwal M M,Kulkarni S R,Arcavi I,et al.PTF 10fqs:A luminous red nova in the spiral galaxy messier 99.Astrophys J,2011,730:134-144
52 Stephenson F R,Green D A.Historical Supernovae and their Remnants,International Series on Astronomy and Astrophysics.Oxford:Clarendon Press,2002
53 Tominaga N,Blinnikov S I,Nomoto K.Supernova explosions of super-asymptotic giant branch stars:Multicolor light curves of electron-capture supernovae.Astrophys J,2013,771:L12
54 van Veelen B.Supernovae Interacting with Their Circumstellar Media.Dissertation for Dcotoral Degree.Utrecht:Utrecht University,2010
55 Schlegel E M,Petre R.A chandra ACIS observation of the X-ray-luminous SN 1988Z.Astrophys J,2006,646:378-384
56 Ibeling D,Heger A.The metallicity dependence of the minimum mass for core-collapse supernovae.Astrophys J,2013,765:L43
57 Jones S,Hirschi R,Nomoto K,et al.Advanced burning stages and fate of 8-10 M⊙stars.Astrophys J,2013,772:150
58 Takahashi K,Yoshida T,Umeda H.Evolution of progenitors for electron capture supernovae.Astrophys J,2013,771:28
59 Poelarends A J T.Stellar Evolution at the Borderline of White Dwarf and Neutron Star Formation.Dissertation for Dcotoral Degree.Utrecht:Utrecht University,2007
60 Langer N,Norman C A,de Koter A,et al.Pair creation supernovae at low and high redshift.Astron Astrophys,2007,475:L19-L23
61 Gal-Yam A,Mazzali P,Ofek E O,et al.Supernova 2007bi as a pair-instability explosion.Nature,2009,462:624-627
62 Ofek E O,Cameron P B,Kasliwal M M,et al.SN 2006gy:An extremely luminous supernova in the galaxy NGC 1260.Astrophys J,2007,659:L13-L16
63 Smith N,Li W,Foley R J,et al.SN 2006gy:Discovery of the most luminous supernova ever recorded,powered by the death of an extremely massive star likeηcarinae.Astrophys J,2007,666:1116-1128
64 Smith N,Chornock R,Silverman J M,et al.Spectral evolution of the extraordinary type iin supernova 2006gy.Astrophys J,2010,709:856-883
65 Quimby R M,Kulkarni S R,Kasliwal M M,et al.Hydrogen-poor superluminous stellar explosions.Nature,2011,474:487-489
66 Arcavi I,Howell D A,Kasen D,et al.Energetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star.Nature,2017,551:210-213
67 Gunn J E,Ostriker J P.On the nature of pulsars.III.Analysis of observations.Astrophys J,1970,160:979
68 Shklovskii I S.Possible causes of the secular increase in pulsar periods.Sov Astron,1970,13:562-565
69 Lyne A G,Lorimer D R.High birth velocities of radio pulsars.Nature,1994,369:127-129
70 Hobbs G,Lorimer D R,Lyne A G,et al.A statistical study of 233 pulsar proper motions.Mon Not R Astron Soc,2005,360:974-992
71 Nordhaus J,Brandt T D,Burrows A,et al.The hydrodynamic origin of neutron star kicks.Mon Not R Astron Soc,2012,423:1805-1812
72 Wongwathanarat A,Janka H T,Müller E.Three-dimensional neutrino-driven supernovae:Neutron star kicks,spins,and asymmetric ejection of nucleosynthesis products.Astron Astrophys,2013,552:A126
73 Kaspi V M,Bailes M,Manchester R N,et al.Evidence from a precessing pulsar orbit for a neutron-star birth kick.Nature,1996,381:584-586
74 Prokhorov M E,Postnov K A.Direct observation of the kick during the birth of a neutron star in the binary pulsar PSR B1259-63.Astron Lett,1997,23:439-444
75 Behroozi P S,Ramirez-Ruiz E,Fryer C L.Interpreting short gamma-ray burst progenitor kicks and time delays using the host galaxy-dark matter halo connection.Astrophys J,2014,792:123-131
76 Pfahl E,Rappaport S,Podsiadlowski P,et al.A new class of high-mass X-ray binaries:Implications for core collapse and neutron star recoil.Astrophys J,2002,574:364-376
77 Corongiu A,Kramer M,Stappers B W,et al.The binary pulsar PSR J1811-1736:Evidence of a low amplitude supernova kick.Astron Astrophys,2007,462:703-709
78 Dewi J D M,Pols O R.The late stages of evolution of helium star-neutron star binaries and the formation of double neutron star systems.Mon Not R Astron Soc,2003,344:629-643
79 Podsiadlowski P,Dewi J D M,Lesaffre P,et al.The double pulsar J0737-3039:Testing the neutron star equation of state.Mon Not R Astron Soc,2005,361:1243-1249
80 Ferdman R D,Stairs I H,Kramer M,et al.The double pulsar:Evidence for neutron star formation without an iron core-collapse supernova.Astrophys J,2013,767:85
81 Guillemot L,Kramer M,Johnson T J,et al.Fermi LAT pulsed detection of PSR J0737-3039A in the double pulsar system.Astrophys J,2013,768:169
82 Burrows A,Hayes J.Pulsar recoil and gravitational radiation due to asymmetrical stellar collapse and explosion.Phys Rev Lett,1996,76:352-355
83 Jonker P G,Nelemans G.The distances to galactic low-mass X-ray binaries:Consequences for black hole luminosities and kicks.Mon Not RAstron Soc,2004,354:355-366
84 Fragos T,Willems B,Ivanova N et al.Black hole formation in X-ray binaries:The case of XTE J1118+48.In:di Salvo T,Israel G L,Piersant L,et al,eds.The Multicolored Landscape of Compact Objects and Their Explosive Origins.American Institute of Physics Conference Proceedings.Toronto,2007.924:673-676
85 Willems B,Henninger M,Levin T,et al.Understanding compact object formation and natal kicks.I.Calculation methods and the case of GROJ1655-40.Astrophys J,2005,625:324-346
86 Kuulkers E,Kouveliotou C,Belloni T,et al.MAXI J1659-152:The shortest orbital period black-hole transient in outburst.Astron Astrophys,2013,552:A32
87 Mirabel I F.Formation of a black hole in the dark.Science,2003,300:1119-1120
88 Wong T W,Valsecchi F,Fragos T,et al.Understanding compact object formation and natal kicks.III.The case of cygnus X-1.Astrophys J,2012,747:111
89 Nelemans G,Tauris T M,van den Heuvel E P J.Constraints on mass ejection in black hole formation derived from black hole X-ray binaries.Astron Astrophys,1999,352:L87-L90
90 Miller-Jones J C A,Jonker P G,Dhawan V,et al.The first accurate parallax distance to a black hole.Astrophys J,2009,706:L230-L234
91 Repetto S,Davies M B,Sigurdsson S.Investigating stellar-mass black hole kicks.Mon Not R Astron Soc,2012,425:2799-2809
92 Lipunov V M,Postnov K A,Prokhorov M E.Formation and coalescence of relativistic binary stars:The effect of kick velocity.Mon Not RAstron Soc,1997,288:245-259
93 Mapelli M,Colpi M,Zampieri L.Low metallicity and ultra-luminous X-ray sources in the cartwheel galaxy.Mon Not R Astron Soc-Lett,2009,395:L71-L75
94 Mapelli M,Zampieri L,Ripamonti E,et al.Dynamics of stellar black holes in young star clusters with different metallicities.I.Implications for X-ray binaries.Mon Not R Astron Soc,2013,429:2298-2314
95 Belczynski K,Bulik T,Fryer C L,et al.On the maximum mass of stellar black holes.Astrophys J,2010,714:1217-1226
96 Fryer C L,Belczynski K,Wiktorowicz G,et al.Compact remnant mass function:dependence on the explosion mechanism and metallicity.Astrophys J,2012,749:91
97 Maeder A.Stellar yields as a function of initial metallicity and mass limit for black hole formation.Astron Astrophys,1992,264:105-120
98 Vink J S,de Koter A,Lamers H J G L M.Mass-loss predictions for O and B stars as a function of metallicity.Astron Astrophys,2001,369:574-588
99 Vink J S,Muijres L E,Anthonisse B,et al.Wind modelling of very massive stars up to 300 solar masses.Astron Astrophys,2011,531:A132
100 Muijres L,Vink J S,de Koter A,et al.Mass-loss predictions for evolved very metal-poor massive stars.Astron Astrophys,2012,546:A42
101 Muijres L E,Vink J S,de Koter A,et al.Predictions for mass-loss rates and terminal wind velocities of massive O-type stars.Astron Astrophys,2012,537:A37
102 Meynet G,Maeder A.Stellar evolution with rotation.XI.Wolf-Rayet star populations at different metallicities.Astron Astrophys,2005,429:581-598
103 Vink J S,de Koter A.On the metallicity dependence of Wolf-Rayet winds.Astron Astrophys,2005,442:587-596
104 Grafener G,Hamann W R.Mass loss from late-type WN stars and its Z-dependence.Very massive stars approaching the Eddington limit.Astron Astrophys,2008,482:945-960
105 Tang J,Bressan A,Rosenfield P,et al.New PARSEC evolutionary tracks of massive stars at low metallicity:Testing canonical stellar evolution in nearby star-forming dwarf galaxies.Mon Not R Astron Soc,2014,445:4287-4305
106 Chen Y,Bressan A,Girardi L,et al.PARSEC evolutionary tracks of massive stars up to 350 M⊙at metallicities 0.0001≤Z≤0.04.Mon Not RAstron Soc,2015,452:1068-1080
107 Muijres L E,de Koter A,Vink J S,et al.Predictions of the effect of clumping on the wind properties of O-type stars.Astron Astrophys,2011,526:A32
108 Vink J S,Grafener G.The transition mass-loss rate:calibrating the role of line-driven winds in massive star evolution.Astrophys J,2012,751:L34
109 Grafener G,Vink J S,de Koter A,et al.The Eddington factor as the key to understand the winds of the most massive stars.Astron Astrophys,2011,535:A56
110 Vink J S.Mass loss and stellar superwinds.Phil Trans R Soc A,2017,375:20160269
111 Bestenlehner J M,Grafener G,Vink J S,et al.The VLT-FLAMES tarantula survey.XVII.Physical and wind properties of massive stars at the top of the main sequence.Astron Astrophys,2014,570:A38
112 Spera M,Mapelli M,Bressan A.The mass spectrum of compact remnants from the PARSEC stellar evolution tracks.Mon Not R Astron Soc,2015,451:4086-4103
113 Spera M,Mapelli M.Very massive stars,pair-instability supernovae and intermediate-mass black holes with the sevn code.Mon Not R Astron Soc,2017,470:4739-4749
114 Giacobbo N,Mapelli M,Spera M.Merging black hole binaries:The effects of progenitor’s metallicity,mass-loss rate and Eddington factor.Mon Not R Astron Soc,2018,474:2959-2974
115 Heger A,Fryer C L,Woosley S E,et al.How massive single stars end their life.Astrophys J,2003,591:288-300
116 Sana H,de Mink S E,de Koter A,et al.Binary interaction dominates the evolution of massive stars.Science,2012,337:444-446
117 Duch?ene G,Kraus A.Stellar multiplicity.Annu Rev Astron Astrophys,2013,51:269-310
118 Reggiani M,Meyer M R.Universality of the companion mass-ratio distribution.Astron Astrophys,2013,553:A124
119 Popova E I,Tutukov A V,Yungelson L R.Study of physical properties of spectroscopic binary stars.Astrophys Space Sci,1982,88:55-80
120 Kouwenhoven M B N,The Primordial Binary Population in the Association Sco OB2.Dissertation for Dcotoral Degree.Amsterdam:University of Amsterdam,2006
121 Kopal Z.Close Binary Systems.The International Astrophysics Series 5.London,New York:Chapman&Hall;Wiley,1959
122 Eggleton P P.Approximations to the radii of Roche lobes.Astrophys J,1983,268:368-369
123 Paczynski B.Gravitational waves and the evolution of close binaries.Acta Astron,1967,17:287-296
124 Hjellming M S,Webbnik R F.Thresholds for rapid mass transfer in binary systems.I.Polytropic models.Astrophys J,1987,318:794-808
125 Hjellming M.Rapid Mass Transfer in Binary Systems.Dissertation for Dcotoral Degree.Urbana-Champaign:University of Illinois at UrbanaChampaign,1989
126 Ge H,Hjellming M S,Webbink R F,et al.Adiabatic mass loss in binary stars.I.Computational method.Astrophys J,2010,717:724-738
127 Ge H,Webbink R F,Chen X,et al.Adiabatic mass loss in binary stars.II.From zero-age main sequence to the base of the giant branch.Astrophys J,2015,812:40
128 Paczynski B,Ziolkowski J,Zytkow A.On the Time-Scale of the Mass Transfer in Close Binaries.In:Hack M,ed.Mass Loss from Stars,Astrophysics and Space Science Library.Berlin Heidelberg:Springer-Verlag,1969.13:237
129 Paczynski B,Sienkiewicz R.Evolution of close binaries VIII.Mass exchange on the dynamical time scale.Acta Astron,1972,22:73-91
130 Soberman G E,Phinney E S,van den Heuvel E P J.Stability criteria for mass transfer in binary stellar evolution.Astron Astrophys,1997,327:620-635
131 Tauris T M,Savonije G J.Formation of millisecond pulsars.I.Evolution of low-mass X-ray binaries with Porb>2 days.Astron Astrophys,1999,350:928-944
132 Podsiadlowski P,Rappaport S,Pfahl E D.Evolutionary sequences for low-and intermediate-mass X-ray binaries.Astrophys J,2002,565:1107-1133
133 Pavlovskii K,Ivanova N.Mass transfer from giant donors.Mon Not R Astron Soc,2015,449:4415-4427
134 Lommen D,Yungelson L,van den Heuvel E,et al.Cygnus X-3 and the problem of the missing Wolf-Rayet X-ray binaries.Astron Astrophys,2005,443:231-241
135 Ghosh K K,Rappaport S,Tennant A F,et al.Discovery of a 3.6 hr eclipsing luminous X-ray binary in the galaxy NGC 4214.Astrophys J,2006,650:872-878
136 Podsiadlowski P,Joss P C,Hsu J J L.Presupernova evolution in massive interacting binaries.Astrophys J,1992,391:246-264
137 Paczynski B.Common envelope binaries.In:Proceedings of Structure and Evolution of Close Binary Systems(IAU Symposium 73)Conference in Cambridge.Cambridge,1975.75-80
138 Yungelson L R.Evolution of the secondary component of a close binary system.Nauchnye Informatsii,1973,27:93
139 Refsdal S,Roth M L,Weigert A.On the binary system AS Eri.Astron Astrophys,1974,36:113-122
140 Webbink R F.The evolution of low-mass close binary systems.IV.0.80M⊙+0.40M⊙catastrophic mass loss.Astrophys J,1977,211:881-889
141 Prialnik D,Livio M.The outcome of accretion on to a fully convective star expansion or contraction?Mon Not R Astron Soc,1985,216:37-52
142 Han Z,Webbink R F.Stability and energetics of mass transfer in double white dwarfs.Astron Astrophys,1999,349:L17-L20
143 Sparks W M,Stecher T P.Supernova:The result of the death spiral of a white dwarf into a red giant.Astrophys J,1974,188:149-153
144 Alexander M E,Chau W Y,Henriksen R N.Orbital evolution of a singly condensed,close binary,by mass loss from the primary and by accretion drag on the condensed member.Astrophys J,1976,204:879-888
145 Ivanova N,Justham S,Chen X,et al.Common envelope evolution:Where we stand and how we can move forward.Astron Astrophys Rev,2013,21:59-131
146 Drake J J,Sarna M J.X-ray evidence of the common envelope phase of V471 tauri.Astrophys J,2003,594:L55-L58
147 Sion E M,Bond H E,Lindler D,et al.Hubble space telescope FUV spectra of the post-common-envelope hyades binary V471 tauri.Astrophys J,2012,751:66
148 Kasliwal M M.Systematically bridging the gap between novae and supernovae.Publ Astron Soc Aust,2012,29:482-488
149 Ivanova N,Justham S,Nandez J L A,et al.Identification of the long-sought common-envelope events.Science,2013,339:433-435
150 Tylenda R,Kaminski T,Udalski A,et al.OGLE-2002-BLG-360:From a gravitational microlensing candidate to an overlooked red transient.Astron Astrophys,2013,555:A16
151 Mac Leod M,Ramirez-Ruiz E.On the accretion-fed growth of neutron stars during common envelope.Astrophys J,2015,798:L19
152 Mac Leod M,Ramirez-Ruiz E.Asymmetric accretion flows within a common envelope.Astrophys J,2015,803:41
153 Mac Leod M,Macias P,Ramirez-Ruiz E,et al.Lessons from the onset of a common envelope episode:The remarkable M31 2015 luminous red nova outburst.Astrophys J,2017,835:282
154 Mac Leod M,Antoni A,Murguia-Berthier A,et al.Common envelope wind tunnel:coefficients of drag and accretion in a simplified context for studying flows around objects embedded within stellar envelopes.Astrophys J,2017,838:56
155 Nandez J L A,Ivanova N,Lombardi Jr J C.Recombination energy in double white dwarf formation.Mon Not R Astron Soc-Lett,2015,450:L39-L43
156 Nandez J L A,Ivanova N.Common envelope events with low-mass giants:Understanding the energy budget.Mon Not R Astron Soc,2016,460:3992-4002
157 Ivanova N,Nandez J L A.Common envelope events with low-mass giants:understanding the transition to the slow spiral-in.Mon Not R Astron Soc,2016,462:362-381
158 Ohlmann S T,Ropke F K,Pakmor R,et al.Hydrodynamic moving-mesh simulations of the common envelope phase in binary stellar systems.Astrophys J,2016,816:L9
159 Ohlmann S T,Roepke F K,Pakmor R,et al.Magnetic field amplification during the common envelope phase.Mon Not R Astron Soc-Lett,2016,462:L121-L125
160 Ohlmann S T,Roepke F K,Pakmor R,et al.Constructing stable 3D hydrodynamical models of giant stars.Astron Astrophys,2017,599:A5
161 Van Den Heuvel E P J.Late stages of close binary systems.Symp-Int Astron Union,1976,73:35-61
162 Tutukov A V,Yungelson L R.Evolution of massive common envelope binaries and mass loss.In:Proceedings of Mass Loss and Evolution of O-type Stars,IAU Symposium 83 in Vancouver Island.Canada,1978.401
163 Webbink R F.Double white dwarfs as progenitors of R Coronae Borealis stars and Type I supernovae.Astrophys J,1984,277:355-360
164 Kashi A,Soker N.A circumbinary disc in the final stages of common envelope and the core-degenerate scenario for Type Ia supernovae.Mon Not R Astron Soc,2011,417:1466-1479
165 Ivanova N,Chaichenets S.Common envelope:Enthalpy consideration.Astrophys J,2011,731:L36-39
166 Ivanova N.Common envelope:On the mass and the fate of the remnant.Astrophys J,2011,730:76
167 Xu X J,Li X D.On the binding energy parameterλof common envelope evolution.Astrophys J,2010,716:114-121
168 De Marco O,Passy J C,Moe M,et al.On theαformalism for the common envelope interaction.Mon Not R Astron Soc,2011,411:2277-2292
169 Davis P J,Kolb U,Knigge C.Is the common envelope ejection efficiency a function of the binary parameters?Mon Not R Astron Soc,2012,419:287-303
170 Zorotovic M,Schreiber M R,Gansicke B T,et al.Post-common-envelope binaries from SDSS.IX:Constraining the common-envelope efficiency.Astron Astrophys,2010,520:A86
171 Davis P J,Kolb U,Willems B.A comprehensive population synthesis study of post-common envelope binaries.Mon Not R Astron Soc,2010,403:179-195
172 Toonen S,Nelemans G.The effect of common-envelope evolution on the visible population of post-common-envelope binaries.Astron Astrophys,2013,557:A87
173 Zorotovic M,Schreiber M R,Garc?a-Berro E,et al.Monte Carlo simulations of post-common-envelope white dwarf+main sequence binaries:The effects of including recombination energy.Astron Astrophys,2014,568:A68
174 Camacho J,Torres S,Garc?a-Berro E,et al.Monte Carlo simulations of post-common-envelope white dwarf+main sequence binaries:Comparison with the SDSS DR7 observed sample.Astron Astrophys,2014,566:A86
175 Nelemans G,Yungelson L R,Portegies Zwart S F,et al.Population synthesis for double white dwarfs.I.Close detached systems.Astron Astrophys,2001,365:491-507
176 Nelemans G,Verbunt F,Yungelson L R,et al.Reconstructing the evolution of double helium white dwarfs:Envelope loss without spiral-in.Astron Astrophys,2000,360:1011-1018
177 Nelemans G,Tout C A.Reconstructing the evolution of white dwarf binaries:Further evidence for an alternative algorithm for the outcome of the common-envelope phase in close binaries.Mon Not R Astron Soc,2005,356:753-764
178 van der Sluys M V,Verbunt F,Pols O R.Modelling the formation of double white dwarfs.Astron Astrophys,2006,460:209-228
179 Gosnell N M,Mathieu R D,Geller A M,et al.Detection of white dwarf companions to blue stragglers in the open cluster NGC 188:Direct evidence for recent mass transfer.Astrophys J,2014,783:L8
180 Gosnell N M,Mathieu R D,Geller A M,et al.Implications for the formation of blue straggler stars from HST ultraviolet observations of NGC188.Astrophys J,2015,814:163
181 Postnov K A,Yungelson L R.The evolution of compact binary star systems.Living Rev Relativ,2014,17:3
182 Flannery B P,van den Heuvel E P J.On the origin of the binary pulsar PSR 1913+16.Astrophys J,1975,39:61-67
183 de Loore C,de Gréve J P,de Cuyper J P.Evolution of massive close binaries.II.The POST X-ray binary stage:Origin of run-away and binary pulsars.Astrophys Space Sci,1975,36:219-225
184 Srinivasan G,van den Heuvel E P J.Some constraints on the evolutionary history of the binary pulsar PSR 1913+16.Astron Astrophys,1982,108:143-147
185 Backer D C,Kulkarni S R,Heiles C,et al.A millisecond pulsar.Nature,1982,300:615-618
186 van den Heuvel E P J.Formation of double neutron stars,millisecond pulsars and double black holes.J Astrophys Astron,2017,38:45.Ar Xiv:1709.07636
187 Tauris T M,Kramer M,Freire P C C,et al.Formation of double neutron star systems.Astrophys J,2017,846:170
188 Nugis T,Lamers H J G L M.Mass-loss rates of Wolf-Rayet stars as a function of stellar parameters.Astron Astrophys,2000,360:227-244
189 Fadeyev Y A,Novikova M F.Radial pulsations of helium stars with masses from 1 to 10 M⊙.Astron Lett,2003,29:522-529
190 Fadeyev Y A,Novikova M F.Radial pulsations of helium stars with masses from 10 to 50M⊙.Astron Lett,2004,30:707-714
191 Miroshnichenko A S.Toward understanding the B[e]phenomenon.I.Definition of the galactic FS CMa stars.Astrophys J,2007,667:497-504
192 Miroshnichenko A S,The B[e]phenomenon:Forty years of studies.Astron Soc Pacific Conf Ser,2017,508:285
193 Khokhlov S A,Miroshnichenko A S,Zharikov S V,et al.Toward understanding the B[e]phenomenon.VII.AS 386,a single-lined binary with a candidate black hole component.Astrophys J,2018,in press.Ar Xiv:1803.03892
194 De Donder E,Vanbeveren D,van Bever J.The number of O-type runaways,the number of O and Wolf-Rayet stars with a compact companion and the formation rate of double pulsars predicted by massive close binary evolution.Astron Astrophys,1997,318:812-818
195 Portegies Zwart S F,Yungelson L R.Formation and evolution of binary neutron stars.Astron Astrophys,1998,332:173-188
196 Kuranov A G,Popov S B,Postnov K A.Pulsar spin-velocity alignment from single and binary neutron star progenitors.Mon Not R Astron Soc,2009,395:2087-2094
197 Ergma E,Yungelson L R,CYG X-3:Can the compact object be a black hole?Astron Astrophys,1998,333:151-158
198 Linden T,Valsecchi F,Kalogera V.On the rarity of X-ray binaries with naked helium donors.Astrophys J,2012,748:114
199 Thorne K S,Zytkow A N.Red giants and supergiants with degenerate neutron cores.Astrophys J,1975,199:L19-L24
200 Barkov M V,Bisnovatyi-Kogan G S,Lamzin S A.The thermal evolution of thorne-zytkow objects.Astron Rep,2001,45:230-235
201 Tout C A,Zytkow A N,Church R P,et al.HV2112,a Thorne-Zytkow object or a super asymptotic giant branch star.Mon Not R Astron Soc-Lett,2014,445:L36-L40
202 Foellmi C,Moffat A F J.Are peculiar wolf-rayet stars of type WN8 Thorne-Zytkow Objects?Astron Soc Pacific Conf Ser,2002,263:123
203 Colgate S A.Neutron-star formation,thermonuclear supernovae,and heavy-element reimplosion.Astrophys J,1971,163:221-230
204 Chevalier R A.Neutron star accretion in a stellar envelope.Astrophys J,1993,411:L33-L36
205 Botticella M T,Smartt S J,Kennicutt Jr R C,et al.A comparison between star formation rate diagnostics and rate of core collapse supernovae within 11 Mpc.Astron Astrophys,2012,537:A132
206 van den Heuvel E P J.X-ray binaries and their descendants:Binary radio pulsars;evidence for three classes of neutron stars?In:Proceedings of5th Integral Workshop On The Integral Universe.ESA Special Publication,2004,552.185
207 Schwab J,Podsiadlowski P,Rappaport S.Further evidence for the bimodal distribution of neutron-star masses.Astrophys J,2010,719:722-727
208 Knigge C,Coe M J,Podsiadlowski P.Two populations of X-ray pulsars produced by two types of supernova.Nature,2011,479:372-375
209 van den Heuvel E P J.Compact stars and the evolution of binary systems.Bull Astrono Soc India,2011,39:1-20
210 Iben I J,Tutukov A V,Yungelson L R.A model of the galactic X-ray binary population.II.Low-mass X-ray binaries in the galactic disk.Astrophys J Suppl Ser,1995,100:233
211 Kalogera V,Webbink R F.Formation of low-mass X-ray binaries.I.Constraints on hydrogen-rich donors at the onset of the X-ray phase.Astrophys J,1996,458:301
212 Kalogera V,Webbink R F.Formation of low-mass X-ray binaries.II.Common envelope evolution of primordial binaries with extreme mass ratios.Astrophys J,1998,493:351-367
213 Tutukov A V,Fedorova A V.Evolution of close stellar binaries with black holes under the action of gravitational radiation and magnetic and induced stellar winds of the donor.Astron Rep,2002,46:765-778
214 Wang B,Podsiadlowski P,Han Z.He-accreting carbon-oxygen white dwarfs and type Ia supernovae.Mon Not R Astron Soc,2017,472:1593-1599
215 Ziosi B M,Mapelli M,Branchesi M,et al.Dynamics of stellar black holes in young star clusters with different metallicities.II.Black hole-black hole binaries.Mon Not R Astron Soc,2014,441:3703-3717
216 Fryer C L.Mass limits for black hole formation.Astrophys J,1999,522:413-418
217 van den Heuvel E P J,Habets G M H J.Observational lower mass limit for black hole formation derived from massive X-ray binaries.Nature,1984,309:598-600
218 Woosley S E,Langer N,Weaver T A.The presupernova evolution and explosion of helium stars that experience mass loss.Astrophys J,1995,448:315-338
219 Portegies Z S F,Verbunt F,Ergma E.The formation of black-holes in low-mass X-ray binaries.Astron Astrophys,1997,321:207-212
220 Ergma E,van den Heuvel E P J.On the initial progenitor masses of stellar mass black holes and neutron stars.Astron Astrophys,1998,331:L29-L32
221 Brown G E,Heger A,Langer N,et al.Formation of high mass X-ray black hole binaries.New Astron,2001,6:457-470
222 Kochanek C S.Failed supernovae explain the compact remnant mass function.Astrophys J,2014,785:28
223 Muno M P,Clark J S,Crowther P A,et al.A neutron star with a massive progenitor in westerlund 1.Astrophys J,2006,636:L41-L44
224 Timmes F X,Woosley S E,Weaver T A.The neutron star and black hole initial mass function.Astrophys J,1996,457:834-843
225 Remillard R A,Mc Clintock J E.X-ray properties of black-hole binaries.Annu Rev Astron Astrophys,2006,44:49-92
226 Fryer C L,Kalogera V.Theoretical black hole mass distributions.Astrophys J,2001,554:548-560
227 Georgy C,Meynet G,Walder R,et al.The different progenitors of type Ib,Ic SNe,and of GRB.Astron Astrophys,2009,502:611-622
228 Linden T,Kalogera V,Sepinsky J F,et al.The effect of starburst metallicity on bright X-ray binary formation pathways.Astrophys J,2010,725:1984-1994
229 Belczynski K,Holz D E,Bulik T,et al.The first gravitational-wave source from the isolated evolution of two stars in the 40-100 solar mass range.Nature,2016,534:512-515
230 Crowther P A,Barnard R,Carpano S,et al.NGC 300 X-1 is a Wolf-Rayet/black hole binary.Mon Not R Astron Soc-Lett,2010,403:L41-L45
231 Foucart F,Deaton M B,Duez M D,et al.Black-hole-neutron-star mergers at realistic mass ratios:Equation of state and spin orientation effects.Phys Rev D,2013,87:084006
232 Endal A S,Sofia S.The evolution of rotating stars.II.Calculations with time-dependent redistribution of angular momentum for 7-and 10-solarmass stars.Astrophys J,1978,220:279-290
233 Zahn J P.Circulation and turbulence in rotating stars.Astron Astrophys,1992,265:115-132
234 Maeder A.Evidences for a bifurcation in massive star evolution.The ON-blue stragglers.Astron Astrophys,1987,178:159-169
235 Woosley S E,Heger A.The progenitor stars of gamma-ray bursts.Astrophys J,2006,637:914-921
236 Brott I,de Mink S E,Cantiello M,et al.Rotating massive main-sequence stars.I.Grids of evolutionary models and isochrones.Astron Astrophys,2011,530:A115
237 Koehler K,Langer N,de Koter A,et al.The evolution of rotating very massive stars with LMC composition.Astron Astrophys,2015,573:A71
238 Szécsi D,Langer N,Yoon S C,et al.Low-metallicity massive single stars with rotation.Evolutionary models applicable to I Zwicky 18.Astron Astrophys,2015,581:A15
239 de Mink S E,Cantiello M,Langer N,et al.Rotational mixing in massive binaries.Detached short-period systems.Astron Astrophys,2009,497:243-253
240 Mandel I,de Mink S E.Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries.Mon Not R Astron Soc,2016,458:2634-2647
241 Song H F,Meynet G,Maeder A,et al.Massive star evolution in close binaries.Conditions for homogeneous chemical evolution.Astron Astrophys,2016,585:A120
242 Marchant P,Langer N,Podsiadlowski P,et al.Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity.Astron Astrophys,2017,604:A55
243 Kilic M,Brown W R,Kenyon S J,et al.The shortest period detached binary white dwarf system.Mon Not R Astron Soc-Lett,2011,413:L101-L105
244 Brown W R,Kilic M,Hermes J J,et al.A 12 minute orbital period detached white dwarf eclipsing binary.Astrophys J,2011,737:L23
245 Hermes J J,Kilic M,Brown W R,et al.Rapid orbital decay in the 12.75-minute binary white dwarf J0651+2844.Astrophys J,2012,757:L21
246 Nelemans G.Galactic Binaries with e LISA.In:Proceedings of the 9th LISA Symposium.Bibliotheque Nationale de France,Paris,2012.ASPConference Series,2013,467.27
247 Brown W R,Kilic M,Prieto C A,et al.The ELM Survey.I.A complete sample of extremely low-mass white dwarfs.Astrophys J,2010,723:1072-1081
248 Kilic M,Brown W R,Prieto C A,et al.The ELM survey.II.Twelve binary white dwarf merger systems.Astrophys J,2011,727:3
249 Brown W R,Kilic M,Allende Prieto C,et al.The ELM survey.III.A successful targeted survey for extremely low mass white dwarfs.Astrophys J,2012,744:142
250 Kilic M,Brown W R,Allende Prieto C,et al.The ELM survey.IV.24 white dwarf merger systems.Astrophys J,2012,751:141
251 Brown W R,Kilic M,Allende Prieto C,et al.The ELM survey.V.Merging massive white dwarf binaries.Astrophys J,2013,769:66
252 Gianninas A,Kilic M,Brown W R,et al.The ELM survey.VI.Eleven new double degenerates.Astrophys J,2015,812:167
253 Brown W R,Gianninas A,Kilic M,et al.The ELM survey.VII.Orbital properties of low-mass white dwarf binaries.Astrophys J,2016,818:155
254 Brown W R,Kilic M,Kenyon S J,et al.Most double degenerate low-mass white dwarf binaries merge.Astrophys J,2016,824:46
255 Kilic M,Hermes J J,Gianninas A,et al.Found:The progenitors of AM CVn and supernovae Ia.Mon Not R Astron Soc-Lett,2014,438:L26-L30
256 Han Z.The formation of double degenerates and related objects.Mon Not R Astron Soc,1998,296:1019-1040
257 Istrate A G,M Tauris T,Langer N.The formation of low-mass helium white dwarfs orbiting pulsars.Evolution of low-mass X-ray binaries below the bifurcation period.Astron Astrophys,2014,571:A45
258 Chen X,Maxted P F L,Li J,et al.The formation of EL CVn-type binaries.Mon Not R Astron Soc,2017,467:1874-1889
259 Han Z,Podsiadlowski P,Maxted P F L,et al.The origin of subdwarf B stars.I.The formation channels.Mon Not R Astron Soc,2002,336:449-466
260 Han Z,Podsiadlowski P,Maxted P F L,et al.The origin of subdwarf B stars.II.Mon Not R Astron Soc,2003,341:669-691
261 Zhang X,Jeffery C S.Evolutionary models for double helium white dwarf mergers and the formation of helium-rich hot subdwarfs.Mon Not RAstron Soc,2012,419:452-464
262 Maoz D,Hallakoun N,Badenes C.The separation distribution and merger rate of double white dwarfs:Improved constraints.Mon Not R Astron Soc,2018,in press.Ar Xiv:1801.04275
263 Solheim J E.AM CVn stars:Status and challenges.Publ Astron Soc Pac,2010,122:1133-1163
264 Pringle J E,Webbink R F.Ariel 1118-61-A very close binary system.Mon Not R Astron Soc,1975,172:493-500
265 Tutukov A V,Yungelson L R.On the influence of emission of gravitational waves on the evolution of low-mass close binary stars.Acta Astron,1979,29:665-680
266 Nelemans G,Yungelson L R,Portegies Zwart S F.The gravitational wave signal from the Galactic disk population of binaries containing two compact objects.Astron Astrophys,2001,375:890-898
267 Zapolsky H S,Salpeter E E.The mass-radius relation for cold spheres of low mass.Astrophys J,1969,158:809-813
268 Nauenberg M.Analytic approximations to the mass-radius relation and energy of zero-temperature stars.Astrophys J,1972,175:417
269 Verbunt F,Rappaport S.Mass transfer instabilities due to angular momentum flows in close binaries.Astrophys J,1988,332:193-198
270 Tutukov A V,Fedorova A V,Formation and evolution of close binaries containing helium donors.Sov Astron,1989,33:606-613
271 Tutukov A,Yungelson L.Double-degenerate semidetached binaries with helium secondaries:Cataclysmic variables,supersoft X-ray sources,supernovae and accretion-induced collapses.Mon Not R Astron Soc,1996,280:1035-1045
272 Nelemans G,Yungelson L R,Portegies Zwart S F.Short-period AM CVn systems as optical,X-ray and gravitational-wave sources.Mon Not RAstron Soc,2004,349:181-192
273 Ruiter A J,Belczynski K,Benacquista M,et al.The LISA gravitational wave foreground:A study of double white dwarfs.Astrophys J,2010,717:1006-1021
274 Deloye C J,Taam R E,Winisdoerffer C,et al.The thermal evolution of the donors in AM canum venaticorum binaries.Mon Not R Astron Soc,2007,381:525-542
275 D’Antona F,Ventura P,Burderi L,et al.Modeling the closest double degenerate system RX J0806.3+1527 and its decreasing period.Astrophys J,2006,653:1429-1434
276 Kaplan D L,Bildsten L,Steinfadt J D R.Orbital evolution of compact white dwarf binaries.Astrophys J,2012,758:64
277 Holcomb C,Guillochon J,De Colle F,et al.Conditions for successful helium detonations in astrophysical environments.Astrophys J,2013,771:14
278 Paczynski B.Evolution of Single Stars.IV.Helium stars.Acta Astron,1971,21:1-14
279 Savonije G J,de Kool M,van den Heuvel E P J.The minimum orbital period for ultra-compact binaries with helium burning secondaries.Astron Astrophys,1986,155:51-57
280 Iben I J,Tutukov A V.Helium star cataclysmics.Astrophys J,1991,370:615-629
281 Ivanova N,Taam R E.Thermal timescale mass transfer and the evolution of white dwarf binaries.Astrophys J,2004,601:1058-1066
282 Yungelson L R.Evolution of low-mass helium stars in semidetached binaries.Astron Lett,2008,34:620-634
283 Fink M,Ropke F K,Hillebrandt W,et al.Double-detonation sub-Chandrasekhar supernovae:Can minimum helium shell masses detonate the core?Astron Astrophys,2010,514:A53
284 Sim S A,Fink M,Kromer M,et al.2D simulations of the double-detonation model for thermonuclear transients from low-mass carbon-oxygen white dwarfs.Mon Not R Astron Soc,2012,420:3003-3016
285 Moll R,Woosley S E.Multi-dimensional models for double detonation in sub-chandrasekhar mass white dwarfs.Astrophys J,2013,774:137
286 Roelofs G H A,Groot P J,Nelemans G,et al.On the orbital periods of the AM CVn stars HP Librae and V803 Centauri.Mon Not R Astron Soc,2007,379:176-182
287 Carter P J,Marsh T R,Steeghs D,et al.A search for the hidden population of AM CVn binaries in the sloan digital sky survey.Mon Not RAstron Soc,2013,429:2143-2160
288 Zhang X F,Liu J Z,Jeffery C S,et al.The double helium-white dwarf channel for the formation of AM CVn binaries.Res Astron Astrophys,2018,18:009
289 Belczynski K,Taam R E.Galactic populations of ultracompact binaries.Astrophys J,2004,603:690-696
290 Miller G E,Scalo J M.The initial mass function and stellar birthrate in the solar neighborhood.Astrophys J Suppl Ser,1979,41:513-547
291 Yungelson L R,Livio M,Tutukov A V,et al.Are the observed frequencies of double degenerates and SN IA contradictory?Astrophys J,1994,420:336-340
292 Nelemans G,Portegies Zwart S F,Verbunt F,et al.Population synthesis for double white dwarfs.II.Semi-detached systems:AM CVn stars.Astron Astrophys,2001,368:939-949
293 Toonen S,Claeys J S W,Mennekens N,et al.Pop CORN:Hunting down the differences between binary population synthesis codes.Astron Astrophys,2014,562:A14
294 Tutukov A V,Yungel Son L R.The merger rate of neutron star and black hole binaries.Mon Not R Astron Soc,1993,260:675-678
295 Lipunov V M,Postnov K A,Prokhorov M E.Black holes and gravitational waves:Possibilities for simultaneous detection using rst-generation laser interferometers.Astron Lett,1997,23:492-497
296 Voss R,Tauris T M.Galactic distribution of merging neutron stars and black holes-prospects for short gamma-ray burst progenitors and LIGO/VIRGO.Mon Not R Astron Soc,2003,342:1169-1184
297 O’Shaughnessy R,Kim C,Fragos T,et al.Constraining population synthesis models via the binary neutron star population.Astrophys J,2005,633:1076-1084
298 Dominik M,Belczynski K,Fryer C,et al.Double compact objects.I.The significance of the common envelope on merger rates.Astrophys J,2012,759:52
299 Mennekens N,Vanbeveren D.Massive double compact object mergers:Gravitational wave sources and r-process element production sites.Astron Astrophys,2014,564:A134
300 Belczynski K,Repetto S,Holz D E,et al.Compact binary merger rates:Comparison with LIGO/Virgo upper limits.Astrophys J,2016,819:108
301 Belczynski K,Heger A,Gladysz W,et al.The effect of pair-instability mass loss on black-hole mergers.Astron Astrophys,2016,594:A97
302 Belczynski K,Ryu T,Perna R,et al.On the likelihood of detecting gravitational waves from Population III compact object binaries.Mon Not RAstron Soc,2017,471:4702-4721
303 Eldridge J J,Stanway E R.BPASS predictions for binary black hole mergers.Mon Not R Astron Soc,2016,462:3302-3313
304 Pavlovskii K,Ivanova N,Belczynski K,et al.Stability of mass transfer from massive giants:Double black hole binary formation and ultraluminous X-ray sources.Mon Not R Astron Soc,2017,465:2092-2100
305 van den Heuvel E P J,Portegies Zwart S F,de Mink S E.Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer.Mon Not R Astron Soc,2017,471:4256-4264
306 Hainich R,Oskinova L M,Shenar T,et al.Observational properties of massive black hole binary progenitors.Astron Astrophys,2018,609:A94
307 Stevenson S,Vigna-Gomez A,Mandel I,et al.Formation of the first three gravitational-wave observations through isolated binary evolution.Nat Commun,2017,8:14906
308 Chruslinska M,Belczynski K,Klencki J,et al.Double neutron stars:Merger rates revisited.Mon Not R Astron Soc,2018,474:2937-2958
309 Vink J S,de Koter A.Predictions of variable mass loss for luminous blue variables.Astron Astrophys,2002,393:543-553
310 Fishbach M,Holz D E.Where are LIGO’s big black holes?Astrophys J,2017,851:L25
311 Kim C,Perera B B P,Mc Laughlin M A.Implications of PSR J0737-3039B for the Galactic NS-NS binary merger rate.Mon Not R Astron Soc,2015,448:928-938
312 Bray J C,Eldridge J J.Neutron star kicks and their relationship to supernovae ejecta mass.Mon Not R Astron Soc,2016,461:3747-3759
313 de Mink S E,Belczynski K.Merger rates of double neutron stars and stellar origin black holes:The impact of initial conditions on binary evolution predictions.Astrophys J,2015,814:58
314 Gupta A,Arun K G,Sathyaprakash B S.Implications of binary black hole detections on the merger rates of double neutron stars and neutron star-black holes.Astrophys J,2017,849:L14
315 de Mink S E,Mandel I.The chemically homogeneous evolutionary channel for binary black hole mergers:Rates and properties of gravitationalwave events detectable by advanced LIGO.Mon Not R Astron Soc,2016,460:3545-3553