Discovery of the correlation between peak episodic jet power and X-ray peak luminosity of the soft state in black hole transients

	Discovery of the correlation between peak episodic jet power and X-ray peak luminosity of the soft state in black hole transients
	Zhang, H.; Yu, W.
刊名	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
	2015-08-01
卷号	451 期号:2 页码:1740-1749
关键词	stars: jets radio continuum: stars X-rays: binaries
英文摘要	Episodic jets are usually observed in the intermediate state of black hole transients during their X-ray outbursts. Here we report the discovery of a strong positive correlation between the peak radio power of the episodic jet P-jet and the corresponding peak X-ray luminosity L-x of the soft state (in Eddington units) in a complete sample of the outbursts of black hole transients observed during the RXTE era of which data are available, which follows the relation log P-jet = (2.2 +/- 0.3) + (1.6 +/- 0.2) x log L-x. The transient ultraluminous X-ray source in M31 and HLX-1 in EXO 243-49 fall on the relation if they contain stellar-mass black hole and either stellar-mass black hole or intermediate-mass black hole, respectively. Besides, a significant correlation between the peak power of the episodic jet and the rate of increase of the X-ray luminosity dL(x)/dt during the rising phase of those outbursts is also found, following log P-jet = (2.0 +/- 0.4) + (0.7 +/- 0.2) x log dL(x)/dt. In GX 339-4 and H 1743-322 in which data for two outbursts are available, measurements of the peak radio power of the episodic jet and the X-ray peak luminosity (and its rate of change) shows similar positive correlations between outbursts, which demonstrate the dominant role of accretion over black hole spin in generating episodic jet power. On the other hand, no significant difference is seen among the systems with different measured black hole spin in current sample. This implies that the power of the episodic jet is strongly affected by non-stationary accretion instead of black hole spin characterized primarily by the rate of change of the mass accretion rate.
WOS标题词	Science & Technology ; Physical Sciences
类目[WOS]	Astronomy & Astrophysics
研究领域[WOS]	Astronomy & Astrophysics
关键词[WOS]	MICROQUASAR XTE J1550-564 ; GX 339-4 ; INFRARED OBSERVATIONS ; LOW/HARD STATE ; RADIO-EMISSION ; 1998 OUTBURST ; GRS 1915+105 ; MULTIPLE EJECTIONS ; RELATIVISTIC JETS ; LIGHT CURVES
收录类别	SCI
语种	英语
WOS记录号	WOS:000360830000048
公开日期	2015-11-10
内容类型	期刊论文
源URL	[http://119.78.226.72/handle/331011/28252]
专题	上海天文台_星系宇宙学重点实验室
作者单位	Chinese Acad Sci, Key Lab Res Galaxies & Cosmol, Shanghai Astron Observ, Shanghai 200030, Peoples R China
推荐引用方式 GB/T 7714	Zhang, H.,Yu, W.. Discovery of the correlation between peak episodic jet power and X-ray peak luminosity of the soft state in black hole transients[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2015,451(2):1740-1749.
APA	Zhang, H.,&Yu, W..(2015).Discovery of the correlation between peak episodic jet power and X-ray peak luminosity of the soft state in black hole transients.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,451(2),1740-1749.
MLA	Zhang, H.,et al."Discovery of the correlation between peak episodic jet power and X-ray peak luminosity of the soft state in black hole transients".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 451.2(2015):1740-1749.