Photometry and spectroscopy of the luminous red nova PSNJ14021678+5426205 in the galaxy M101

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• 作者：V. P. Goranskij ; E. A. Barsukova ; O. I. Spiridonova ; A. F. Valeev…
• 关键词：novae ; cataclysmic variables ; binaries ; close ; stars ; individual ; PSNJ14021678+5426205
• 刊名：Astrophysical Bulletin
• 出版年：2016
• 出版时间：January 2016
• 年：2016
• 卷：71
• 期：1
• 页码：82-94
• 全文大小：1,127 KB
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• 作者单位：V. P. Goranskij (1)
  E. A. Barsukova (2)
  O. I. Spiridonova (2)
  A. F. Valeev (2) (3)
  T. A. Fatkhullin (2)
  A. S. Moskvitin (2)
  O. V. Vozyakova (1)
  D. V. Cheryasov (1)
  B. S. Safonov (1)
  A. V. Zharova (1)
  T. Hancock (4)
  
  1. Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, 119991, Russia
  2. Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, 369167, Russia
  3. Kazan Federal University, Kazan, 420008, Russia
  4. Down Under Observatory, Fremont, MI, USA
  
• 刊物类别：Physics and Astronomy
• 刊物主题：Physics
  Astronomy, Astrophysics and Cosmology
  Russian Library of Science
  
• 出版者：MAIK Nauka/Interperiodica distributed exclusively by Springer Science+Business Media LLC.
• ISSN：1990-3421

文摘

We present the results of the study of a red nova from the observations carried out with the Russian 6-m telescope (BTA) along with other telescopes of SAO RAS and SAI MSU. To investigate the nova progenitor,we used the data from the Digital Sky Survey and amateur photos available on the Internet. In the period between April 1993 and July 2014, the brightness of the progenitor gradually increased by \(2_ \cdot ^m 2\) in the V-band. At the peak of the first outburst in mid-November 2014, the star reached an absolute visual magnitude of \(- 12_ \cdot ^m 75\) but was discovered later, in February 2015, in a repeated outburst at the magnitude of \(- 11_ \cdot ^m 65\). The amplitude of the outburst was minimum among the red novae, only \(5_ \cdot ^m 6\) in V-band. The Hα emission line and the background of a cool supergiant continuum with gradually decreasing surface temperature were observed in the spectra. Such process is typical for red novae, although the object under study showed extreme parameters: maximum luminosity, maximum outburst duration, minimum outburst amplitude, unusual shape of the light curve. This event is interpreted as a massive OB star system components’merging accompanied by formation of a common envelope and then the expansion of this envelope with minimal energy losses.