RELATIONSHIP BETWEEN THE KINETIC POWER AND BOLOMETRIC LUMINOSITY OF JETS: LIMITATION FROM BLACK HOLE X-RAY BINARIES, ACTIVE GALACTIC NUCLEI, AND GAMMA-RAY BURSTS

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	RELATIONSHIP BETWEEN THE KINETIC POWER AND BOLOMETRIC LUMINOSITY OF JETS: LIMITATION FROM BLACK HOLE X-RAY BINARIES, ACTIVE GALACTIC NUCLEI, AND GAMMA-RAY BURSTS
	Ma, Renyi ; Xie, Fu-Guo ; Hou, Shujin ; Ma RY(马任意)
刊名	http://dx.doi.org/10.1088/2041-8205/780/1/L14
	2014
关键词	RELATIVISTIC JETS ACCRETION RATE RADIO-SOURCES HARD STATES EMISSION GALAXIES ORIGIN SHOCKS CANDIDATES EVOLUTION
英文摘要	Natural Science Foundation of China [11333004, 11203057, 11133005, 11233006, 11103059, 11103061, 11121062]; CAS/SAFEA International Partnership Program for Creative Research Teams; Natural Science Foundation of Fujian Province [2011J01023]; The correlation between the kinetic power P-jet and intrinsic bolometric luminosity L-jet of jets may reveal the underlying jet physics in various black hole systems. Based on the recent work by Nemmen et al., we re-investigate this correlation with additional sources of black hole X-ray binaries (BXBs) in hard/quiescent states and low-luminosity active galactic nuclei (LLAGNs). The new sample includes 29 sets of data from 7 BXBs and 20 LLAGNs, with P-jet and L-jet being derived from spectral modeling of the quasi-simultaneous multi-band spectra under the accretion jet scenario. Compared to previous works, the range of luminosity is now enlarged to more than 20 decades, i.e., from similar to 10(31) erg s(-1) to similar to 10(52) erg s(-1), which allows for better constraining of the correlation. One notable result is that the jets in BXBs and LLAGNs almost follow the same P-jet-L-jet correlation that was obtained from blazars and gamma-ray bursts. The slope indices we derived are 1.03+/-0.01 for the whole sample, 0.85+/-0.06 for the BXB subsample, 0.71+/-0.11 for the LLAGN subsample, and 1.01+/-0.05 for the LLAGN-blazar subsample, respectively. The correlation index around unit implies the independence of jet efficiency on the luminosity or kinetic power. Our results may further support the hypothesis that similar physical processes exist in the jets of various black hole systems.
语种	英语
出版者	IOP PUBLISHING LTD
内容类型	期刊论文
源URL	[http://dspace.xmu.edu.cn/handle/2288/92106]
专题	物理技术－已发表论文
推荐引用方式 GB/T 7714	Ma, Renyi,Xie, Fu-Guo,Hou, Shujin,et al. RELATIONSHIP BETWEEN THE KINETIC POWER AND BOLOMETRIC LUMINOSITY OF JETS: LIMITATION FROM BLACK HOLE X-RAY BINARIES, ACTIVE GALACTIC NUCLEI, AND GAMMA-RAY BURSTS[J]. http://dx.doi.org/10.1088/2041-8205/780/1/L14,2014.
APA	Ma, Renyi,Xie, Fu-Guo,Hou, Shujin,&马任意.(2014).RELATIONSHIP BETWEEN THE KINETIC POWER AND BOLOMETRIC LUMINOSITY OF JETS: LIMITATION FROM BLACK HOLE X-RAY BINARIES, ACTIVE GALACTIC NUCLEI, AND GAMMA-RAY BURSTS.http://dx.doi.org/10.1088/2041-8205/780/1/L14.
MLA	Ma, Renyi,et al."RELATIONSHIP BETWEEN THE KINETIC POWER AND BOLOMETRIC LUMINOSITY OF JETS: LIMITATION FROM BLACK HOLE X-RAY BINARIES, ACTIVE GALACTIC NUCLEI, AND GAMMA-RAY BURSTS".http://dx.doi.org/10.1088/2041-8205/780/1/L14 (2014).