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Constraining the radio jet proper motion of the high-redshift quasar J2134-0419 at z=4.3
Perger, Krisztina1,2; Frey, Sandor2; Gabanyi, Krisztina E.2,3; An, Tao4,5; Britzen, Silke6; Cao, Hong-Min7,8; Cseh, David2; Dennett-Thorpe, Jane9; Gurvits, Leonid, I10,11; Hong, Xiao-Yu4,5; Hook, Isobel M.12; Paragi, Zsolt10; Schilizzi, Richard T.13; Yang, Jun4,14; Zhang, Yingkang4
2018-06-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume477Issue:1Pages:1065-1070
Contribution Rank8
Abstract

To date, PMN J2134-0419 (at a redshift z = 4.33) is the second most distant quasar known with a milliarcsecond-scale morphology permitting direct estimates of the jet proper motion. Based on two-epoch observations, we constrained its radio jet proper motion using the very long baseline interferometry (VLBI) technique. The observations were conducted with the European VLBI Network (EVN) at 5 GHz on 1999 November 26 and 2015 October 6. We imaged the central 10-pc scale radio jet emission and modelled its brightness distribution. By identifying a jet component at both epochs separated by 15.86 yr, a proper motion of mu = 0.035 +/- 0.023 mas yr(-1) is found. It corresponds to an apparent superluminal speed of beta(a)= 4.1 +/- 2.7 c. Relativistic beaming at both epochs suggests that the jet viewing angle with respect to the line of sight is smaller than 20 degrees, with a minimum bulk Lorentz factor Gamma = 4.3. The small value of the proper motion is in good agreement with the expectations from the cosmological interpretation of the redshift and the current cosmological model. Additionally we analysed archival Very Large Array observations of J2143-0419 and found indication of a bent jet extending to similar to 30 kpc.

KeywordGalaxies: Active Galaxies: High-redshift Galaxies: Nuclei Quasars: Individual: Pmn J2134-0419 Radio Continuum: Galaxies
SubtypeArticle
DOI10.1093/mnras/sty837
WOS HeadingsScience & Technology ; Physical Sciences
URL查看原文
Indexed BySCI
Language英语
WOS KeywordActive Galactic Nuclei ; Source Catalog ; Vlbi Survey ; Sky Survey ; Kinematics ; Cosmology ; Galaxies ; Sample
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000432660300076
Funding OrganizationEVN(ES034, EC054) ; Hungarian National Research, Development, and Innovation Office(OTKA NN110333) ; International Cooperation Bureau of the Chinese Academy of Sciences ; Hungarian Academy of Sciences ; program of the Light in China's Western Region(2016-QNXZ-B-21) ; National Science Foundation of China(U1731103, 11573016)
Citation statistics
Cited Times:3[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/1926
Collection其它
Corresponding AuthorPerger, Krisztina
Affiliation1.Eotvos Lorand Univ, Dept Astron, Pazmany Peter Setany 1-A, H-1117 Budapest, Hungary
2.MTA Res Ctr Astron & Earth Sci, Konkoly Observ, Konkoly Thege Miklos Ut 15-17, H-1121 Budapest, Hungary
3.MTA ELTE Extragalact Astrophys Res Grp, Pazmany Peter Setany 1-A, H-1117 Budapest, Hungary
4.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
5.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China
6.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
7.Shangqiu Normal Univ, Sch Elect & Elect Engn, Wenhua Rd 298, Shangqiu 476000, Henan, Peoples R China
8.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
9.Univ Manchester, Manchester M13 9PL, Lancs, England
10.Joint Inst VLBI ERIC, POB 2, NL-7990 AA Dwingeloo, Netherlands
11.Delft Univ Technol, Dept Astrodynam & Space Missions, Kluyverweg 1, NL-2629 HS Delft, Netherlands
12.Univ Lancaster, Dept Phys, Lancaster LA1 4YB, England
13.Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Manchester M13 9PL, Lancs, England
14.Chalmers Univ Technol, Dept Space Earth & Environm, Onsala Space Observ, SE-43992 Onsala, Sweden
Recommended Citation
GB/T 7714
Perger, Krisztina,Frey, Sandor,Gabanyi, Krisztina E.,et al. Constraining the radio jet proper motion of the high-redshift quasar J2134-0419 at z=4.3[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,477(1):1065-1070.
APA Perger, Krisztina.,Frey, Sandor.,Gabanyi, Krisztina E..,An, Tao.,Britzen, Silke.,...&Zhang, Yingkang.(2018).Constraining the radio jet proper motion of the high-redshift quasar J2134-0419 at z=4.3.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,477(1),1065-1070.
MLA Perger, Krisztina,et al."Constraining the radio jet proper motion of the high-redshift quasar J2134-0419 at z=4.3".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 477.1(2018):1065-1070.
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