Institutional Repository of Radio Astronomy Research Laboratory
On the Difference of Quasars and BL Lac Objects | |
Liu, Xiang![]() | |
2009-08-01 | |
Conference Name | Workshop on Approaching Micro-Arcsecond Resolution with VSOP-2 |
Source Publication | Approaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technologies ASP Conference Series |
Volume | 402 |
Pages | 307-309 |
Conference Date | DEC 03-07, 2007 |
Conference Place | Inst Space & Astronaut Sci, Kanagawa, JAPAN |
Country | JAPAN |
Publisher | Astronomical Soc Pacific |
Contribution Rank | 1 |
Abstract | We analyze the two differences between radio-loud quasars and BL Lacs: the lack of emission lines in BL Lacs, and the different position angles of the jets. We propose that BL Lacs have much less gas and are possibly optically-thin near the central engine in nuclei. This could be attributed to the orbiting of binary black holes in a very late merging stage. |
URL | 查看原文 |
Indexed By | CPCI |
Language | 英语 |
ISBN | 978-1-58381-679-0 |
WOS ID | WOS:000270005100066 |
Citation statistics | |
Document Type | 会议论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/4150 |
Collection | 射电天文研究室_星系宇宙学研究团组 |
Affiliation | Urumqi Observatory of NAOC, 40-5 South Beijing Rd, Urumqi 830011, China |
First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Recommended Citation GB/T 7714 | Liu, Xiang. On the Difference of Quasars and BL Lac Objects[C]:Astronomical Soc Pacific,2009:307-309. |
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Liu-2009-On the Diff(59KB) | 会议论文 | 开放获取 | CC BY-NC-SA | View Application Full Text |
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