Intrinsic gamma-ray luminosity, black hole mass, jet and accretion in Fermi blazars

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	Intrinsic gamma-ray luminosity, black hole mass, jet and accretion in Fermi blazars
	Xiong DR(熊定荣)1,2 ; Zhang, X3
刊名	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
	2014-07-11
卷号	441 期号:4 页码:3375-3395
关键词	radiation mechanisms: non-thermal galaxies: active BL Lacertae objects: general quasars: general gamma-rays: general X-rays: general
ISSN号	0035-8711
通讯作者	Xiong, DR (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
产权排序	第一完成单位
英文摘要	We have analysed a large sample of clean blazars detected by Fermi Large Area Telescope (LAT). Using the literature and calculation, we obtained intrinsic gamma-ray luminosity excluding beaming effect, black hole mass, broad-line luminosity (used as a proxy for disc luminosity), jet kinetic power from 'cavity' power and bulk Lorentz factor for parsec-scale radio emission, and studied the distributions of these parameters and relations between them. Our main results are as follows. (i) After excluding beaming effect and redshift effect, intrinsic gamma-ray luminosity with broad-line luminosity, black hole mass and Eddington ratio have significant correlations. Our results confirm the physical distinction between BL Lacs and FSRQs. (ii) The correlation between broad-line luminosity and jet power is significant which supports that jet power has a close link with accretion. Jet power depends on both the Eddington ratio and black hole mass. We also obtain logL(BLR) similar to (0.98 +/- A 0.07)logP(jet) for all blazars, which is consistent with the theoretical predicted coefficient. These results support that jets are powered by energy extraction from both accretion and black hole spin (i.e. not by accretion only). (iii) For almost all BL Lacs, P-jet > L-disc; for most of FSRQs, P-jet < L-disc. The 'jet-dominance' (parametrized as P-jet/L-disc) is mainly controlled by the bolometric luminosity. Finally, the radiative efficiency of gamma-ray and properties of TeV blazars detected by Fermi LAT were discussed.
学科主题	Astronomy & Astrophysics
WOS标题词	Science & Technology ; Physical Sciences
类目[WOS]	Astronomy & Astrophysics
研究领域[WOS]	Astronomy & Astrophysics
关键词[WOS]	ACTIVE GALACTIC NUCLEI ; BL-LACERTAE OBJECTS ; LARGE-AREA TELESCOPE ; RADIO-LOUD QUASARS ; TEV BLAZARS ; X-RAY ; LAC OBJECTS ; PHYSICAL-PROPERTIES ; ENERGY-DISTRIBUTION ; INFRARED RADIATION
收录类别	SCI
原文出处	http://mnras.oxfordjournals.org/content/441/4/3375
语种	英语
WOS记录号	WOS:000338764700041
内容类型	期刊论文
源URL	[http://ir.ynao.ac.cn/handle/114a53/4250]
专题	云南天文台_其他
作者单位	1.National Astronomical Observatories/Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China 2.The Graduate School of Chinese Academy of Sciences, Beijing 100049, China 3.Department of Physics, Yunnan Normal University, Kunming 650500, China
推荐引用方式 GB/T 7714	Xiong DR,Zhang, X. Intrinsic gamma-ray luminosity, black hole mass, jet and accretion in Fermi blazars[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2014,441(4):3375-3395.
APA	Xiong DR,&Zhang, X.(2014).Intrinsic gamma-ray luminosity, black hole mass, jet and accretion in Fermi blazars.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,441(4),3375-3395.
MLA	Xiong DR,et al."Intrinsic gamma-ray luminosity, black hole mass, jet and accretion in Fermi blazars".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 441.4(2014):3375-3395.