Profile of an emission line from relativistic outflows around a black hole | |
Wang JM(王建民)![]() ![]() ![]() | |
刊名 | ASTROPHYSICAL JOURNAL
![]() |
2000 | |
卷号 | 544期号:1页码:381-389 |
关键词 | black hole physics line : profiles relativity |
通讯作者 | Acad Sinica, Inst High Energy Phys, Lab Cosm Ray & High Energy Astrophys, Beijing 100039, Peoples R China ; Peking Univ, Chinese Acad Sci, Beijing Astrophys Ctr, Beijing 100871, Peoples R China ; Univ Sci & Technol China, Ctr Astrophys, Hefei 230026, Peoples R China ; Chinese Acad Sci, Natl Astron Observ, Beijing 100864, Peoples R China ; Chinese Acad Sci, Shanghai Observ, Shanghai 200019, Peoples R China |
英文摘要 | Recent observations show strong evidence for the presence of Doppler-shifted emission lines in the spectrum of both black hole candidates and active galactic nuclei. These lines are likely to originate from relativistic outflows (or jets) in the vicinity of the central black: hole. Consequently, the profile of such a line should be distorted by strong gravitational effects near the black hole, as well as special relativistic effects. In this paper, we present results from a detailed study on how each process affects the observed line profile. We found that the profile is sensitive to the intrinsic properties of the jets (Lorentz factor, velocity profile, and emissivity law), as well as to the spin of the black hole and the viewing angle (with respect to the axis of the jets). More specifically, in the case of approaching jets, an intrinsically narrow line (blueshifted) is seen as simply broadened at small viewing angles, but it shows a doubly peaked profile at large viewing angles for extreme Kerr black holes (due to the combination of gravitational focusing and Doppler effects); the profile is always singly peaked for Schwarzschild black holes. For receding jets, however, the line profile becomes quite complicated owing to complicated photon trajectories. To facilitate comparison with observations, we searched a large parameter space to derive representative line profiles. We show the results and discuss how to use emission lines as a potential tool for probing the inner region of a black hole jet system. |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
原文出处 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000165751300033 |
内容类型 | 期刊论文 |
源URL | [http://ir.ihep.ac.cn/handle/311005/237249] ![]() |
专题 | 高能物理研究所_粒子天体物理中心 高能物理研究所_多学科研究中心 |
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 | Wang JM,Wu M,Wang, JM,et al. Profile of an emission line from relativistic outflows around a black hole[J]. ASTROPHYSICAL JOURNAL,2000,544(1):381-389. |
APA | 王建民.,吴枚.,Wang, JM.,Zhou, YY.,Yuan, YF.,...&Wu, M.(2000).Profile of an emission line from relativistic outflows around a black hole.ASTROPHYSICAL JOURNAL,544(1),381-389. |
MLA | 王建民,et al."Profile of an emission line from relativistic outflows around a black hole".ASTROPHYSICAL JOURNAL 544.1(2000):381-389. |
个性服务 |
查看访问统计 |
相关权益政策 |
暂无数据 |
收藏/分享 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论