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Jet opening angle and linear scale of launch region of blazars
Liu, Xiang1,2; Jiang, Pengfei1,3; Cui, Lang1,4
2021-01-29
Conference NameProceedings of the International Astronomical Union , Volume 15 , Symposium S356: Nuclear Activity in Galaxies Across Cosmic Time
Source PublicationProceedings of the International Astronomical Union , Volume 15 , Symposium S356: Nuclear Activity in Galaxies Across Cosmic Time 
Volume15
IssueS356
Pages320-322
Conference Date7-11 October 2019
Conference PlaceAddis Ababa, Ethiopia
CountryEthiopia
Author of SourceMirjana Pović et al.
Contribution Rank1
AbstractWe explore the intrinsic jet opening angle (IJOA) of blazars, from the literature, we found that the blazar number density peaks around 0.5° of IJOA and declines quickly with increasing IJOA for flat spectrum radio quasars (FSRQs), while the number density has double peaks around 0.3° and 2.0° of IJOA for BL Lacs. We assume that the black hole accretion-produced jet may have the smaller IJOA (for its larger linear scale of launch region), and the BH spin-produced jet may have the larger IJOA (for its smaller launch region), such that the FSRQs are accretion dominated for their single peaked small IJOA, while the BL Lacs are either accretion or BH spin dominated for their double peaked IJOA.
KeywordGalaxies: jets quasars: general BL Lacertae objects: general
DOI10.1017/S1743921320003221
URL查看原文
Indexed By其他
Language英语
ISSN1743-9213
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Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/4667
Collection射电天文研究室_星系宇宙学研究团组
Corresponding AuthorLiu, Xiang
Affiliation1.Xinjiang Astronomical Observatory, CAS, 150 Science-1 Street, Urumqi 830011, China;
2.Qiannan Normal University for Nationalities, 558000 Duyun, China;
3.Graduate University of Chinese Academy of Sciences, Beijing 100049, China;
4.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China
Recommended Citation
GB/T 7714
Liu, Xiang,Jiang, Pengfei,Cui, Lang. Jet opening angle and linear scale of launch region of blazars[C]//Mirjana Pović et al.,2021:320-322.
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