中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The obstructed jet in Mrk 231

文献类型:期刊论文

作者Wang, Ailing2,3; An, Tao3; Jaiswal, Sumit3; Mohan, Prashanth3; Wang, Yuchan3; Baan, Willem A.1,3; Zhang, Yingkang3; Yang, Xiaolong3
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2021-07-01
卷号504期号:3页码:3823-3830
ISSN号0035-8711
关键词galaxies: ISM galaxies: jets galaxies: kinematics and dynamics quasars: individual (Mrk 231)
DOI10.1093/mnras/stab587
通讯作者An, Tao(antao@shao.ac.cn)
英文摘要Mrk 231 is the closest radio-quiet quasar known and one of the most luminous infrared galaxies in the local Universe. It is characterized by the co-existence of a radio jet and powerful multiphase multiscale outflows, making it an ideal laboratory to study active galactic nucleus (AGN) feedback. We analyse the multi-epoch very long baseline interferometry data of Mrk 231 and estimate the jet head advance speed to be less than or similar to 0.013 c, suggesting a sub-relativistic jet flow. The jet position angle changes from -113. in the inner parsec to -172 degrees at a projected distance of 25 pc. The jet structure change might result from either a jet bending following the rotation of the circum-nuclear disc or the projection of a helical jet on the plane of the sky. In the large opening angle (similar to 60 degrees) cone, the curved jet interacts with the interstellar medium and creates wide-aperture-angle shocks that subsequently dissipate a large portion of the jet power through radiation and contribute to powering the large-scale outflows. The low power and bent structure of the Mrk 231 jet, as well as extensive radiation dissipation, are consistent with the obstruction of the short-length jet by the host galaxy's environment.
WOS关键词BINARY BLACK-HOLE ; ACTIVE GALACTIC NUCLEUS ; RADIO JET ; ULTRAVIOLET-SPECTRUM ; VLBA OBSERVATIONS ; KILOPARSEC-SCALE ; RELATIVISTIC JET ; ABSORPTION ; GALAXY ; OUTFLOWS
资助项目National Key R&D Programme of China[2018YFA0404603] ; Chinese Academy of Sciences (CAS)[114231KYSB20170003] ; CAS-PIFI[2020PM0057]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000656139300047
资助机构National Key R&D Programme of China ; Chinese Academy of Sciences (CAS) ; CAS-PIFI
源URL[http://ir.xao.ac.cn/handle/45760611-7/4544]  
专题新疆天文台_射电天文研究室
通讯作者An, Tao
作者单位1.Chinese Acad Sci, Xinjiang Astron Observ, Key Lab Radio Asimn, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
2.Univ Chinese Acad Sci, Sch Astron & Space Sci, 19A Yuquanlu, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Radio Astron, 80 Nandan Rd, Shanghai 200030, Peoples R China
推荐引用方式
GB/T 7714
Wang, Ailing,An, Tao,Jaiswal, Sumit,et al. The obstructed jet in Mrk 231[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2021,504(3):3823-3830.
APA Wang, Ailing.,An, Tao.,Jaiswal, Sumit.,Mohan, Prashanth.,Wang, Yuchan.,...&Yang, Xiaolong.(2021).The obstructed jet in Mrk 231.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,504(3),3823-3830.
MLA Wang, Ailing,et al."The obstructed jet in Mrk 231".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 504.3(2021):3823-3830.

入库方式: OAI收割

来源:新疆天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。