The jets-accretion relation, mass-luminosity relation in Fermi blazars

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• 作者：Xiaoling Yu (1)
  Xiong Zhang (1)
  Haojing Zhang (1)
  Dingrong Xiong (1)
  Bijun Li (1)
  Yongjuan Cha (1)
  Yongyun Chen (1)
  Xia Huang (1)
  Yuwei Wang (1)
  
  1. Department of Physics ; Yunnan Normal University ; 650500 ; Kunming ; China
  
• 关键词：Accretion ; accretion disk ; Galaxies ; jets ; Galaxies ; evolution ; Quasars ; general
• 刊名：Astrophysics and Space Science
• 出版年：2015
• 出版时间：May 2015
• 年：2015
• 卷：357
• 期：1
• 全文大小：600 KB
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• 刊物类别：Physics and Astronomy
• 刊物主题：Physics
  Astronomy
  
• 出版者：Springer Netherlands
• ISSN：1572-946X

文摘

A sample of 111 Fermi blazars each with a well-established radio core luminosity, broad-line luminosity, bolometric luminosity and black hole mass has been compiled from the literatures. We present a significant correlation between radio core and broad-line emission luminosities that supports a close link between accretion processes and relativistic jets. Analysis reveals a relationship of \(\mathrm{Log}\mathrm{L}_{\mathrm{BLR}}\sim(0.81\pm0.06)\mathrm{Log} \mathrm{L}_{\mathrm{R}}^{\mathrm{C}}\) which is consistant with theoretical predicted coefficient and supports that blazar jets are powered by energy extraction from a rapidly spinning Kerr black hole through the magnetic field provided by the accretion disk. Through studying the correlation between the intrinsic bolometric luminosity and the black hole mass, we find a relationship of \(\mathrm{Log}\frac{\mathrm{L}_{\mathrm{in}}}{\mathrm{L}_{\odot}}=(0.95\pm0.26)\mathrm{Log} \frac{\mathrm{M}}{\mathrm{M}_{\odot}}+(3.53\pm2.24)\) which supports mass-luminosity relation for Fermi blazars derived in this work is a powerlaw relation similar to that for main-sequence stars. Finally, EVOLUTIONARY SEQUENCE OF BLAZARS is discussed.