A timing view of the heartbeat state of GRS 1915+105

doi:10.1093/mnras/stw2916

	A timing view of the heartbeat state of GRS 1915+105
	Yan, Shu-Ping 1,2,3; Ji, Li1,2 ; Mendez, Mariano 4; Liu, Si-Ming1,2 ; Wang, Na 5; Li, Xiang-Dong 3,6; Ge, Ming-Yu 7; Liao, Jin-Yuan 7; Niu, Shu 1,2; Qu, Jin-Lu 7
刊名	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
	2017-02-01
卷号	465 期号:2 页码:1926-1933
关键词	accretion, accretion discs black hole physics X-rays: binaries X-rays: individual GRS 1915+105
ISSN号	0035-8711
DOI	10.1093/mnras/stw2916
通讯作者	Yan, Shu-Ping(yanshuping@pmo.ac.cn)
英文摘要	We present a timing analysis of two Rossi X-ray Timing Explorer observations of the micro-quasar GRS 1915+ 105 during the heartbeat state. The phase-frequency-power maps show that the intermediate-frequency aperiodic X-ray variability weakens as the source softens in the slow rise phase, and when the quasi-periodic oscillation disappears in the rise phase of the pulse of the double-peaked class, its sub-harmonic is still present with a hard phase lag. In the slow rise phase, the energy-frequency-power maps show that most of the aperiodic variability is produced in the corona, and may also induce the aperiodic variability observed at low energies from an accretion disc, which is further supported by the soft phase lag especially in the intermediate-frequency range (with a time delay up to 20 ms). In the rise phase of the pulse, the low-frequency aperiodic variability is enhanced significantly and there is a prominent hard lag (with a time delay up to 50 ms), indicating that the variability is induced by extension of the disc towards small radii as implied by the increase in flux and propagates into the corona. However, during the hard pulse of the double-peaked class, the variability shows no significant lag, which may be attributed to an optically thick corona. These timing results are generally consistent with the spectral results presented by Neilsen, Remillard & Lee which indicated that the slow rise phase corresponds to a local Eddington limit and the rise phase of the pulse corresponds to a radiation pressure instability in the disc.
WOS关键词	QUASI-PERIODIC OSCILLATIONS ; BLACK-HOLE CANDIDATES ; X-RAY BINARIES ; TIME-LAGS ; PHASE-LAG ; XTE J1550-564 ; CYGNUS X-1 ; GRS-1915+105 ; FREQUENCY ; VARIABILITY
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	OXFORD UNIV PRESS
WOS记录号	WOS:000393785500047
内容类型	期刊论文
源URL	[http://libir.pmo.ac.cn/handle/332002/23285]
专题	中国科学院紫金山天文台
通讯作者	Yan, Shu-Ping
作者单位	1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 2.Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Nanjing 210008, Jiangsu, Peoples R China 3.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Jiangsu, Peoples R China 4.Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands 5.Chinese Acad Sci, Xinjiang Astron Observ, Xinjiang 830011, Peoples R China 6.Nanjing Univ, Dept Astron, Nanjing 210093, Jiangsu, Peoples R China 7.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
推荐引用方式 GB/T 7714	Yan, Shu-Ping,Ji, Li,Mendez, Mariano,et al. A timing view of the heartbeat state of GRS 1915+105[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,465(2):1926-1933.
APA	Yan, Shu-Ping.,Ji, Li.,Mendez, Mariano.,Liu, Si-Ming.,Wang, Na.,...&Sun, Wei.(2017).A timing view of the heartbeat state of GRS 1915+105.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,465(2),1926-1933.
MLA	Yan, Shu-Ping,et al."A timing view of the heartbeat state of GRS 1915+105".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 465.2(2017):1926-1933.