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On the Difference of Quasars and BL Lac Objects
Liu, Xiang
2009-08-01
Conference NameWorkshop on Approaching Micro-Arcsecond Resolution with VSOP-2
Source PublicationApproaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technologies ASP Conference Series
Volume402
Pages307-309
Conference DateDEC 03-07, 2007
Conference PlaceInst Space & Astronaut Sci, Kanagawa, JAPAN
CountryJAPAN
PublisherAstronomical Soc Pacific
Contribution Rank1
AbstractWe 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.
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Indexed ByCPCI
Language英语
ISBN978-1-58381-679-0
WOS IDWOS:000270005100066
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type会议论文
Identifierhttp://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
AffiliationUrumqi Observatory of NAOC, 40-5 South Beijing Rd, Urumqi 830011, China
First Author AffilicationXinjiang 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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