MODELING THE HARD STATES OF THREE BLACK HOLE CANDIDATES
文献类型:期刊论文
| 作者 | Zhang, Hui1,2 ; Yuan, Feng1 ; Chaty, Sylvain3
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2010-07-10 |
| 卷号 | 717期号:2页码:929-936 |
| 关键词 | accretion accretion disks black hole physics ISM: jets and outflows stars: individual (SWIFT J1753.5-0127 GRO J1655-40 XTE J1720-319) |
| 英文摘要 | Simultaneous multiwavelength observations were recently performed for three black hole candidates-SWIFT J1753.5-0127, GRO J1655-40, and XTE J1720-318. In this paper, we test the accretion-jet model originally proposed for XTE J1118+480 by investigating the hard state of these three sources using this model. The accretion flow in the model is composed of an inner hot accretion flow and an outer truncated thin disk. We find that the model satisfactorily explains the spectrum ranging from radio to X-rays, with the radio and X-ray spectra dominated by the synchrotron and thermal Comptonization emissions in the jet and the hot accretion flow, respectively, with the infrared and optical being the sum of the emissions from the jet, hot accretion flow, and the truncated thin disk. Similar to the case of XTE J1118+480, the model can also explain, although only qualitatively in some cases, the observed timing features including quasi-periodic oscillation, and positive and negative time lags between the optical and X-ray emissions detected in SWIFT J1753.5-0127. The origin of the ejection events detected in XTE J1720-318 is also briefly discussed. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | X-RAY TRANSIENT ; ADVECTION-DOMINATED ACCRETION ; BROAD-BAND SPECTRUM ; INNER COOL DISKS ; LOW/HARD-STATE ; XTE J1118+480 ; SWIFT J1753.5-0127 ; GRO J1655-40 ; FUNDAMENTAL PLANE ; 2005 OUTBURST |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000280650800026 |
| 公开日期 | 2011-06-29 |
| 源URL | [http://119.78.226.72//handle/331011/13365] ![]() |
| 专题 | 上海天文台_星系宇宙学重点实验室 |
| 作者单位 | 1.Chinese Acad Sci, Key Lab Res Galaxies & Cosmol, Shanghai Astron Observ, Shanghai 200030, Peoples R China 2.Chinese Acad Sci, Grad Sch, Beijing 100039, Peoples R China 3.Univ Paris 07, CEA, CEA Saclay, Serv Astrophys,DSM,IRFU,CNRS,UMR 7158, FR-91191 Gif Sur Yvette, France |
| 推荐引用方式 GB/T 7714 | Zhang, Hui,Yuan, Feng,Chaty, Sylvain. MODELING THE HARD STATES OF THREE BLACK HOLE CANDIDATES[J]. ASTROPHYSICAL JOURNAL,2010,717(2):929-936. |
| APA | Zhang, Hui,Yuan, Feng,&Chaty, Sylvain.(2010).MODELING THE HARD STATES OF THREE BLACK HOLE CANDIDATES.ASTROPHYSICAL JOURNAL,717(2),929-936. |
| MLA | Zhang, Hui,et al."MODELING THE HARD STATES OF THREE BLACK HOLE CANDIDATES".ASTROPHYSICAL JOURNAL 717.2(2010):929-936. |
入库方式: OAI收割
来源:上海天文台
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