A timing view of the heartbeat state of GRS 1915+105
文献类型：期刊论文
| 作者 | Qu JL(屈进禄) ; Yan, SP; Ji, L; Mendez, M; Liu, SM; Wang, N; Li, XD; Ge, MY; Liao, JY; Niu, S
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| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| 出版日期 | 2017 |
| 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 |
| 文献子类 | Article |
| 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. |
| 电子版国际标准刊号 | 1365-2966 |
| 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 |
| WOS记录号 | WOS:000393785500047 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/284848]  |
| 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 |
| 推荐引用方式 GB/T 7714 | Qu JL,Yan, SP,Ji, L,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 | 屈进禄.,Yan, SP.,Ji, L.,Mendez, M.,Liu, SM.,...&廖进元.(2017).A timing view of the heartbeat state of GRS 1915+105.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,465(2),1926-1933. |
| MLA | 屈进禄,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. |
入库方式： OAI收割
来源：高能物理研究所
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