%0 Generic %1 citeulike:13593038 %A Yu, Xiaoling %A Zhang, Xiong %A Zhang, Haojing %A Xiong, Dingrong %A Li, Bijun %A Cha, Yongjuan %A Chen, Yongyun %A Huang, Xia %A Wang, Yuwei %D 2015 %K imported %T The jets-accretion relation, mass-luminosity relation in Fermi blazars %U http://arxiv.org/abs/1504.05635 %X 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 \$LogL\_BLR\sim(0.81\pm0.06)LogL\_R^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 \$LogL\_inL\_ødot=(0.95\pm0.26)LogMM\_ødot+(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.

@misc{citeulike:13593038, abstract = {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 \$\rm{LogL\_{BLR}\sim(0.81\pm0.06)LogL\_{R}^{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 \$\rm{{Log}\frac{L\_{in}}{L\_{\odot}}=(0.95\pm0.26){Log}\frac{M}{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.}, added-at = {2019-03-25T08:20:55.000+0100}, archiveprefix = {arXiv}, author = {Yu, Xiaoling and Zhang, Xiong and Zhang, Haojing and Xiong, Dingrong and Li, Bijun and Cha, Yongjuan and Chen, Yongyun and Huang, Xia and Wang, Yuwei}, biburl = {https://www.bibsonomy.org/bibtex/298ad908bae1e4b6b3b4d5d059024ac6f/ericblackman}, citeulike-article-id = {13593038}, citeulike-linkout-0 = {http://arxiv.org/abs/1504.05635}, citeulike-linkout-1 = {http://arxiv.org/pdf/1504.05635}, day = 22, eprint = {1504.05635}, interhash = {e53ebe47a73d5db44717d98f30ab6b77}, intrahash = {98ad908bae1e4b6b3b4d5d059024ac6f}, keywords = {imported}, month = apr, posted-at = {2015-04-27 09:31:37}, priority = {2}, timestamp = {2019-03-25T08:20:55.000+0100}, title = {{The jets-accretion relation, mass-luminosity relation in Fermi blazars}}, url = {http://arxiv.org/abs/1504.05635}, year = 2015 }