中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Disc-corona interaction in the heartbeat state of GRS 1915+105

文献类型:期刊论文

作者Mendez, M; Li, XD; Qu, JL; Yan, SP; Ji, L; Sun, W; Ge, MY; Liao, JY; Niu, S; Ding, GQ
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2018
卷号474期号:1页码:1214-1224
关键词accretion, accretion discs black hole physics X-rays: binaries X-rays: individual: GRS 1915+105
ISSN号0035-8711
DOI10.1093/mnras/stx2885
文献子类Article
英文摘要Timing analysis provides information about the dynamics of matter accreting on to neutron stars and black holes, and hence is crucial for studying the physics of the accretion flow around these objects. It is difficult, however, to associate the different variability components with each of the spectral components of the accretion flow. We apply several new methods to two Rossi X-ray Timing Explorer observations of the black hole binary GRS 1915+105 during its heartbeat state to explore the origin of the X-ray variability and the interactions of the accretion-flow components. We offer a promising window into the disc-corona interaction through analysing the formation regions of the disc aperiodic variabilities with different time-scales via comparing the corresponding transition energies of the amplitude-ratio spectra. In a previous paper, we analysed the Fourier power density as a function of energy and frequency to study the origin of the aperiodic variability, and combined that analysis with the phase lag as a function of frequency to derive a picture of the disc-corona interaction in this source. We here, for the first time, investigate the phase-lag as a function of energy and frequency, and display some interesting details of the disc-corona interaction. Besides, the results from the shape of amplitude-ratio spectrum and from several other aspects suggest that the quasi-periodic oscillation originates from the corona.
电子版国际标准刊号1365-2966
WOS关键词X-RAY BINARIES ; QUASI-PERIODIC OSCILLATIONS ; ACCRETING BLACK-HOLES ; ADVECTION-DOMINATED ACCRETION ; POWER SPECTRA ; FAST VARIABILITY ; NEUTRON-STARS ; 4TH EDITION ; HARD STATE ; CYGNUS X-1
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000424339500086
源URL[http://ir.ihep.ac.cn/handle/311005/285633]  
专题高能物理研究所_粒子天体物理中心
高能物理研究所_理论物理室
作者单位中国科学院高能物理研究所
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GB/T 7714
Mendez, M,Li, XD,Qu, JL,et al. Disc-corona interaction in the heartbeat state of GRS 1915+105[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,474(1):1214-1224.
APA Mendez, M.,Li, XD.,Qu, JL.,Yan, SP.,Ji, L.,...&Wang, N.(2018).Disc-corona interaction in the heartbeat state of GRS 1915+105.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,474(1),1214-1224.
MLA Mendez, M,et al."Disc-corona interaction in the heartbeat state of GRS 1915+105".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 474.1(2018):1214-1224.

入库方式: OAI收割

来源:高能物理研究所

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