The X-ray view of black-hole candidate Swift J1842.5-1124 during its 2008 outburst
文献类型：期刊论文
| 作者 | Zhao, HH; Weng SS(翁山杉); Qu JL(屈进禄) ; Weng, SS; Qu, JL; Cai, JP; Yuan, QR
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| 刊名 | ASTRONOMY & ASTROPHYSICS
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| 出版日期 | 2016 |
| 卷号 | 593 |
| 关键词 | accretion, accretion disks black hole physics X-rays: stars X-rays: individuals: Swift J1842.5-1124 X-rays: binaries |
| DOI | 10.1051/0004-6361/201628647 |
| 英文摘要 | Context. The spectral and temporal evolution during X-ray outbursts give important clues on the accretion process and radiation mechanism in black-hole X-ray binaries (BH XRBs). Aims. A set of Swift and RXTE observations were executed to monitor the 2008 outburst of the black-hole candidate Swift J1842.5-1124. We investigate these data to explore the accretion physics in BH XRBs. Methods. We carry out a comprehensive spectral and timing analysis on all the available pointing observations, including fitting both X-ray spectra and power density spectra, measuring the optical and near-ultraviolet flux density. We also search for correlations among the spectral and timing parameters. Results. The observed properties of Swift J1842.5-1124 are similar to other BH XRBs in many respects, for example the hardness-intensity diagram and hardness-rms diagram. The type-C quasi-periodic oscillations (QPOs) were observed as the source started to transit from the low-hard state to the high-soft state. The frequency of QPOs correlate with intensity and the hard component index, and anti-correlate with the hardness and the total fractional rms. These relations are consistent with the Lense-Thirring precession model. The estimated U-band flux changed with the X-ray flux, while the flux density at the V-band remained 0.26 mJy. These results imply that the X-ray reprocessing or the tail of thermal emission from the outer disk contributes a significant fraction of the U-band radiation; alternatively, the companion star or the jet dominates the flux at longer wavelengths. |
| 语种 | 英语 |
| WOS记录号 | WOS:000385820100097 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/260703]  |
| 专题 | 中国科学院高能物理研究所 |
| 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 | Zhao, HH,Weng SS,Qu JL,et al. The X-ray view of black-hole candidate Swift J1842.5-1124 during its 2008 outburst[J]. ASTRONOMY & ASTROPHYSICS,2016,593. |
| APA | Zhao, HH.,翁山杉.,屈进禄.,Weng, SS.,Qu, JL.,...&Yuan, QR.(2016).The X-ray view of black-hole candidate Swift J1842.5-1124 during its 2008 outburst.ASTRONOMY & ASTROPHYSICS,593. |
| MLA | Zhao, HH,et al."The X-ray view of black-hole candidate Swift J1842.5-1124 during its 2008 outburst".ASTRONOMY & ASTROPHYSICS 593(2016). |
入库方式： OAI收割
来源：高能物理研究所
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