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题名: The VLBI structure of radio-loud Broad Absorption Line quasars
作者: Liu Yi(刘怡)1, 3; Jiang, D. R.2, 3; Gu, M.2
刊名: ASTRONOMISCHE NACHRICHTEN
出版日期: 2016-02-01
卷号: 337, 期号:1-2, 页码:184-187
关键词: galaxies: active ; galaxies: jets ; quasars: absorption lines ; quasars: general ; techniques: high angular resolution
DOI: 10.1002/asna.201512291
文章类型: Article
英文摘要: The nature and origin of Broad Absorption Line (BAL) quasars and their relationship to non-BAL quasars are an open question. The BAL quasars are probably normal quasars seen along a particular line of sight. Alternatively, they are young or recently refueled. The high resolution radio morphology of BAL quasars is very important to understand the radio properties of BAL quasars. We present VLBA observations at L and C bands for a sample of BAL quasars. The observations will help us to explore the VLBI radio properties, and distinguish the present models of explaining BAL phenomena. (C) 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
WOS标题词: Science & Technology ; Physical Sciences
类目[WOS]: Astronomy & Astrophysics
研究领域[WOS]: Astronomy & Astrophysics
关键词[WOS]: POLARIZATION PROPERTIES ; SPECTRUM
收录类别: SCI
项目资助者: European Commission(283393) ; Natural Science Foundation of China(11233006) ; Chinese Academy of Sciences(XDB09030400) ; National Science Foundation of China(11473054 ; Science and Technology Commission of Shanghai Municipality(14ZR1447100) ; (BK20131460) ; U1531245)
语种: 英语
WOS记录号: WOS:000370147600031
Citation statistics:
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/16132
Appears in Collections:分子云与恒星形成研究团组_期刊论文

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作者单位: 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
2.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, 80 Nandan Rd, Shanghai 200030, Peoples R China
3.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China
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