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Role of the companion lensing galaxy in the CLASS gravitational lens B1152+199
Zhang, M.1,2; Yuan, Q.1,3; Liu, J-Y1,3; Zhang, L.4
2022-02-04
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume511Issue:1Pages:1085-1103
Contribution Rank1
AbstractWe reinvestigate the Cosmic Lens All-Sky Survey (CLASS) gravitational lens B1152+199 using archived Hubble Space Telescope (HST) data and Very Long Baseline Interferometry (VLBI) data. A consistent luminosity ratio within effective radius between the host galaxy and the X-galaxy is measured from HST tri-band images, which leads to a mass ratio between the two galaxies as r(b) similar to 2. To determine the role of the X-galaxy in the lens system, we modelled the dual-lens system with constraints from the VLBI-resolved jet components and the HST images. The 8.4-GHz global-VLBI data currently provide the most stringent constraints to the mass model, especially to the radial power-law slope. The optimized models for this two-image three-component radio lens favour a steeper-than-isothermal inner slope. The jet bending in image B was also investigated and it turned out to be rather a misalignment than a curvature. The goodness-of-fit indicates that the role of the X-galaxy is crucial in the lens system if three pairs of resolved jet components are to be fitted. When we imported the optimal model from radio constraints to optical modelling with the HST tri-band data, the optimization kept the consistency of the optimal model and successfully reproduced the features observed in the HST images. This implies that the diffuse emission discovered in the HST images is actually a detection of the secondary lensing effects from the companion lens.
Keywordgravitational lensing: strong galaxies: jets galaxies: structure dark matter
DOI10.1093/mnras/stac087
Indexed BySCI
Language英语
WOS KeywordDARK-MATTER SUBSTRUCTURE ; EDGE-ON DISC ; MASS SUBSTRUCTURE ; ACS SURVEY ; SYSTEM ; SHARP ; RADIO ; DECOMPOSITION ; UNIVERSALITY ; B1422+231
Funding ProjectNational Science Foundation of China[12173078] ; National Science Foundation of China[11773062] ; West Light Foundation of Chinese Academy of Sciences[2017-XBQNXZ-A-008] ; EVN project[BB133] ; EVN project[GJ010] ; EVN project[BW084] ; EVN project[GA036] ; NASA[NAS 5-26555]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000770034100006
PublisherOXFORD UNIV PRESS
Funding OrganizationNational Science Foundation of China ; West Light Foundation of Chinese Academy of Sciences ; EVN project ; NASA
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Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/4532
Collection中国科学院新疆天文台
Corresponding AuthorZhang, M.
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 831001, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Peoples R China
3.Univ Chinese Acad Sci, 19A Liequan Rd, Beijing 100049, Peoples R China
4.Guizhou Univ, Coll Big Data & Informat Engn, Guiyang 550025, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhang, M.,Yuan, Q.,Liu, J-Y,et al. Role of the companion lensing galaxy in the CLASS gravitational lens B1152+199[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2022,511(1):1085-1103.
APA Zhang, M.,Yuan, Q.,Liu, J-Y,&Zhang, L..(2022).Role of the companion lensing galaxy in the CLASS gravitational lens B1152+199.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,511(1),1085-1103.
MLA Zhang, M.,et al."Role of the companion lensing galaxy in the CLASS gravitational lens B1152+199".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 511.1(2022):1085-1103.
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