KMS of Xinjiang Astronomical Observatory, CAS
| The variability classes in IGR J17091-3624 during the 2011 outburst | |
Zhang, Z.1,2 ; Qu, J. L.1; Gao, H. Q.1,2; Zhang, S.1; Bu, Q. C.3; Ge, M. Y.1; Chen, L.3; Li, Z. B.4
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| 2014-09-01 | |
| Source Publication | ASTRONOMY & ASTROPHYSICS
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| Volume | 569Pages:A33 |
| Contribution Rank | 4 |
| Abstract | Aims. Based on the Rossi X-ray Timing Explorer (RXTE) data, we studied the typical variability classes in IGR J17091-3624 during the 2011 outburst and attempted to understand the physical mechanism that produces the highly structured variability. Methods. Using the rate-resolved spectroscopy, we produced color-color diagrams (CCDs), hardness-intensity diagrams (HIDs), and rate-resolved energy spectra for each class. The time lags were calculated by means of the cross-power spectrum (CPS) analysis. Results. Our study provides a comprehensive understanding of the nu, rho, alpha, beta/lambda, mu and gamma classes during this outburst. The source shows up with different track directions in the CCD loops and different types of the lag at similar to 1-6 s which are class dependent. It is notable that each variability class showing hard lags presents an anti-clockwise loop in the CCD, while each variability class showing soft lags presents a clockwise loop in the CCD. We discuss these observational results with the current models proposed for this type of system. The observed hardness ratio shows an increasing trend toward the high disk temperature for different classes, which can be regarded as evidence for thermal-viscous instability. |
| Keyword | Stars: Individual: Igr J17091-3624 X-rays: Binaries Black Hole Physics Accretion Accretion Disks |
| Subtype | Article |
| DOI | 10.1051/0004-6361/201323294 |
| WOS Headings | Science & Technology ; Physical Sciences |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | BLACK-HOLE CANDIDATE ; QUASI-PERIODIC OSCILLATIONS ; X-RAY BINARIES ; GRS 1915+105 ; EVOLUTION ; MODEL |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000343092100031 |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/582 |
| Collection | 已撤销研究室/团组_高能天体物理研究团组 射电天文研究室 |
| Affiliation | 1.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China 4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China |
| Recommended Citation GB/T 7714 | Zhang, Z.,Qu, J. L.,Gao, H. Q.,et al. The variability classes in IGR J17091-3624 during the 2011 outburst[J]. ASTRONOMY & ASTROPHYSICS,2014,569:A33. |
| APA | Zhang, Z..,Qu, J. L..,Gao, H. Q..,Zhang, S..,Bu, Q. C..,...&Li, Z. B..(2014).The variability classes in IGR J17091-3624 during the 2011 outburst.ASTRONOMY & ASTROPHYSICS,569,A33. |
| MLA | Zhang, Z.,et al."The variability classes in IGR J17091-3624 during the 2011 outburst".ASTRONOMY & ASTROPHYSICS 569(2014):A33. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| The variability clas（750KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-ND | View Application Full Text | |
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