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VLBI astrometry on the white dwarf pulsar AR Scorpii
Jiang, Pengfei1,2; Cui, Lang1,3; Yang, Jun4; Zhang, Bo5; Xu, Shuangjing5,6; Shu, Fengchun5; Jiang, Wu5; Chen, Wen2,7; Li, Guanghui1; Xia, Bo5; Weston, Stuart8; Gulyaev, Sergei8; Cao, Hongmin9; Liu, Xiang1,3; An, Tao1,5
2023-02-01
Source PublicationMonthly Notices of the Royal Astronomical Society
ISSN0035-8711
Volume520Issue:2Pages:2942-2951
Contribution Rank1
AbstractAR Scorpii (AR Sco), the only-known radio-pulsing white dwarf binary, shows unusual pulsating emission at the radio, infrared, optical, and ultraviolet bands. To determine its astrometric parameters at the radio band independently, we conducted multi-epoch Very Long Baseline Interferometry (VLBI) phase-referencing observations with the European VLBI Network at 5 GHz and the Chinese VLBI Network plus the Warkworth 30-m telescope (New Zealand) at 8.6 GHz. By using the differential VLBI astrometry, we provide high-precision astrometric measurements on the parallax (pi = 8.52(-0.07)(+0.04) mas) and proper motion (mu(alpha) = 9.48(-0.07)(+0.04) mas yr(-1), mu(delta) = -51.32(-0.38)(+0.22) mas yr (-1)). The new VLBI results agree with the optical Gaia astrometry. Our kinematic analysis reveals that the Galactic space velocities of AR Sco are quite consistent with that of both intermediate polars and polars. Combined with the previous tightest VLBI constraint on the size, our parallax distance suggests that the radio emission of AR Sco should be located within the light cylinder of its white dwarf.
Keywordtechniques: high angular resolution parallaxes pulsars: individual: AR Sco white dwarfs radio continuum: stars x-ray optical observations emission geometry radio-emission black-hole binary mass sco kinematics herculis Astronomy & Astrophysics
SubtypeArticle
DOI10.1093/mnras/stad327
Indexed BySCI
Language英语
WOS IDWOS:000941753400005
Citation statistics
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/6642
Collection射电天文研究室_星系宇宙学研究团组
科研仪器设备产出_利用南山26米射电望远镜(NSRT)观测数据的文章
Corresponding AuthorCui, Lang
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, 830011 Urumqi, P. R. China;
2.School of Astronomy and Space Science, University of Chinese Academy of Sciences, 100049 Beijing, P. R. China;
3.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, 150 Science 1-Street, 830011 Urumqi, P. R. China;
4.Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, Sweden;
5.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, P. R. China;
6.Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea;
7.Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, Yunnan, P.R. China;
8.Institute for Radio Astronomy and Space Research, A uc kland University of Technology, Private Bag 92006, A uc kland 1142, New Zealand;
9.School of Electronic and Electrical Engineering, Shangqiu Normal University, Wenhua Road 298, Shangqiu, Henan 476000, P. 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
Jiang, Pengfei,Cui, Lang,Yang, Jun,et al. VLBI astrometry on the white dwarf pulsar AR Scorpii[J]. Monthly Notices of the Royal Astronomical Society,2023,520(2):2942-2951.
APA Jiang, Pengfei.,Cui, Lang.,Yang, Jun.,Zhang, Bo.,Xu, Shuangjing.,...&An, Tao.(2023).VLBI astrometry on the white dwarf pulsar AR Scorpii.Monthly Notices of the Royal Astronomical Society,520(2),2942-2951.
MLA Jiang, Pengfei,et al."VLBI astrometry on the white dwarf pulsar AR Scorpii".Monthly Notices of the Royal Astronomical Society 520.2(2023):2942-2951.
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