RELATIONSHIP BETWEEN THE KINETIC POWER AND BOLOMETRIC LUMINOSITY OF JETS: LIMITATION FROM BLACK HOLE X-RAY BINARIES, ACTIVE GALACTIC NUCLEI, AND GAMMA-RAY BURSTS
文献类型：期刊论文
| 作者 | Ma, Renyi1,2; Xie, Fu-Guo3; Hou, Shujin1,2,4 |
| 刊名 | ASTROPHYSICAL JOURNAL LETTERS
 |
| 出版日期 | 2014 |
| 卷号 | 780期号:1页码:0 |
| ISSN号 | 2041-8205 |
| 关键词 | accretion, accretion disks galaxies: jets gamma-ray burst: general ISM: jets and outflows X-rays: binaries |
| 英文摘要 | The correlation between the kinetic power P-jet and intrinsic bolometric luminosity L-jet of jets may reveal the underlying jet physics in various black hole systems. Based on the recent work by Nemmen et al., we re-investigate this correlation with additional sources of black hole X-ray binaries (BXBs) in hard/quiescent states and low-luminosity active galactic nuclei (LLAGNs). The new sample includes 29 sets of data from 7 BXBs and 20 LLAGNs, with P-jet and L-jet being derived from spectral modeling of the quasi-simultaneous multi-band spectra under the accretion jet scenario. Compared to previous works, the range of luminosity is now enlarged to more than 20 decades, i.e., from similar to 10(31) erg s(-1) to similar to 10(52) erg s(-1), which allows for better constraining of the correlation. One notable result is that the jets in BXBs and LLAGNs almost follow the same P-jet-L-jet correlation that was obtained from blazars and gamma-ray bursts. The slope indices we derived are 1.03+/-0.01 for the whole sample, 0.85+/-0.06 for the BXB subsample, 0.71+/-0.11 for the LLAGN subsample, and 1.01+/-0.05 for the LLAGN-blazar subsample, respectively. The correlation index around unit implies the independence of jet efficiency on the luminosity or kinetic power. Our results may further support the hypothesis that similar physical processes exist in the jets of various black hole systems. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | RELATIVISTIC JETS ; ACCRETION RATE ; RADIO-SOURCES ; HARD STATES ; EMISSION ; GALAXIES ; ORIGIN ; SHOCKS ; CANDIDATES ; EVOLUTION |
| 收录类别 | SCI |
| 原文出处 | 10.1088/2041-8205/780/1/L14 |
| 语种 | 英语 |
| WOS记录号 | WOS:000328261500014 |
| 公开日期 | 2014-11-20 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/10660]  |
| 专题 | 紫金山天文台_太阳活动的多波段观测研究团组 |
| 作者单位 | 1.Xiamen Univ, Dept Astron, Xiamen 361005, Fujian Province, Peoples R China 2.Xiamen Univ, Inst Theoret Phys & Astrophys, Xiamen 361005, Fujian Province, Peoples R China 3.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China 4.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China |
| 推荐引用方式 GB/T 7714 | Ma, Renyi,Xie, Fu-Guo,Hou, Shujin. RELATIONSHIP BETWEEN THE KINETIC POWER AND BOLOMETRIC LUMINOSITY OF JETS: LIMITATION FROM BLACK HOLE X-RAY BINARIES, ACTIVE GALACTIC NUCLEI, AND GAMMA-RAY BURSTS[J]. ASTROPHYSICAL JOURNAL LETTERS,2014,780(1):0. |
| APA | Ma, Renyi,Xie, Fu-Guo,&Hou, Shujin.(2014).RELATIONSHIP BETWEEN THE KINETIC POWER AND BOLOMETRIC LUMINOSITY OF JETS: LIMITATION FROM BLACK HOLE X-RAY BINARIES, ACTIVE GALACTIC NUCLEI, AND GAMMA-RAY BURSTS.ASTROPHYSICAL JOURNAL LETTERS,780(1),0. |
| MLA | Ma, Renyi,et al."RELATIONSHIP BETWEEN THE KINETIC POWER AND BOLOMETRIC LUMINOSITY OF JETS: LIMITATION FROM BLACK HOLE X-RAY BINARIES, ACTIVE GALACTIC NUCLEI, AND GAMMA-RAY BURSTS".ASTROPHYSICAL JOURNAL LETTERS 780.1(2014):0. |
入库方式： OAI收割
来源：紫金山天文台
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