PMO OpenIR  > 分子云与恒星形成研究团组
The VLBI structure of radio-loud Broad Absorption Line quasars
Liu, Y.1,3; Jiang, D. R.2,3; Gu, M.2
2016-02-01
Source PublicationASTRONOMISCHE NACHRICHTEN
Volume337Issue:1-2Pages:184-187
AbstractThe 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
KeywordGalaxies: Active Galaxies: Jets Quasars: Absorption Lines Quasars: General Techniques: High Angular Resolution
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1002/asna.201512291
WOS KeywordPOLARIZATION PROPERTIES ; SPECTRUM
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000370147600031
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Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/16132
Collection分子云与恒星形成研究团组
Affiliation1.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
Recommended Citation
GB/T 7714
Liu, Y.,Jiang, D. R.,Gu, M.. The VLBI structure of radio-loud Broad Absorption Line quasars[J]. ASTRONOMISCHE NACHRICHTEN,2016,337(1-2):184-187.
APA Liu, Y.,Jiang, D. R.,&Gu, M..(2016).The VLBI structure of radio-loud Broad Absorption Line quasars.ASTRONOMISCHE NACHRICHTEN,337(1-2),184-187.
MLA Liu, Y.,et al."The VLBI structure of radio-loud Broad Absorption Line quasars".ASTRONOMISCHE NACHRICHTEN 337.1-2(2016):184-187.
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