What Governs Lorentz Factors of Jet Components in Blazars?
文献类型：期刊论文
| 作者 | Cao, XW1; Chai, B2; Zhou M(周明)3 ; Gu, MF1
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| 刊名 | JOURNAL OF ASTROPHYSICS AND ASTRONOMY
 |
| 出版日期 | 2014-09 |
| 卷号 | 35期号:3页码:357-362 |
| 关键词 | Black hole physics accretion galaxies: jets |
| ISSN号 | 0250-6335 |
| 产权排序 | 第三完成单位 |
| 通讯作者 | Cao, XW (reprint author), Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, 80 Nandan Rd, Shanghai 200030, Peoples R China. |
| 英文摘要 | We use a sample of radio-loud Active Galactic Nuclei (AGNs) with measured black hole masses to explore the jet formation mechanisms in these sources. We find a significant correlation between black hole mass and the bulk Lorentz factor of the jet components for this sample, while no significant correlation is present between the bulk Lorentz factor and the Eddington ratio. Recent investigations suggested that the most super-massive black holes in elliptical galaxies have on average higher spins than the black holes in spiral galaxies. The correlation between black hole mass and bulk Lorentz factor of the jet components found in this work implies that the motion velocity of the jet components is probably governed by the black hole spin. The faster moving jets are magnetically accelerated by the magnetic fields threading the horizon of more rapidly rotating black holes. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | ACTIVE GALACTIC NUCLEI ; RADIO-LOUD QUASARS ; RELATIVISTIC JETS ; LINE EMISSION ; BLACK-HOLES |
| 收录类别 | SCI |
| 原文出处 | http://link.springer.com/article/10.1007%2Fs12036-014-9230-z |
| 语种 | 英语 |
| WOS记录号 | WOS:000350481700036 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/5038]  |
| 专题 | 云南天文台_高能天体物理研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
| 作者单位 | 1.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, 200030, China 2.Polar Research Institute of China, 451 Jinqiao Road, Pudong, Shanghai, 200136, China 3.Key Laboratory for the Structure and Evolution of Celestial Objects, Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, China |
| 推荐引用方式 GB/T 7714 | Cao, XW,Chai, B,Zhou M,et al. What Governs Lorentz Factors of Jet Components in Blazars?[J]. JOURNAL OF ASTROPHYSICS AND ASTRONOMY,2014,35(3):357-362. |
| APA | Cao, XW,Chai, B,Zhou M,&Gu, MF.(2014).What Governs Lorentz Factors of Jet Components in Blazars?.JOURNAL OF ASTROPHYSICS AND ASTRONOMY,35(3),357-362. |
| MLA | Cao, XW,et al."What Governs Lorentz Factors of Jet Components in Blazars?".JOURNAL OF ASTROPHYSICS AND ASTRONOMY 35.3(2014):357-362. |
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来源：云南天文台
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