中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
4FGL J1318.2+6754: A Long Orbital-period Redback Candidate

文献类型:期刊论文

作者Lin, Jie2,3,4; Chen HL(陈海亮)1,6; Wang, Bojun5; Xu, Renxin2,3,4
刊名ASTROPHYSICAL JOURNAL LETTERS
出版日期2024
卷号960期号:1
ISSN号2041-8205
DOI10.3847/2041-8213/ad1580
产权排序第4完成单位
文献子类Article
英文摘要By combining the Fermi catalog and the single-lined spectroscopic binaries of Gaia Data Release 3 (DR3), we report a new candidate redback millisecond pulsar binary, which is recommended as a target for radio telescopes to detect pulsed signals. Using TESS data in the T band spanning over 4 yr, we find a period of similar to 4.13 days, which is consistent with the radial velocity solution of the Gaia DR3 and optical spectroscopy from the LAMOST telescope. The light curve in the T band reveals periodic modulation of low amplitude that is a characteristic feature of the heating of the photosphere of a nondegenerate low-mass stellar companion by the pulsar wind. The nondegenerate companion is a bright (G = 11.96), slightly metal-poor ([Fe/H] = - 0.55), G-type main-sequence star (T eff = 5891 K; logg=4.07; R = 1.356R circle dot). This orbital period of 4.13 days would be the longest one for known redback candidates, which could hardly be understood for its formation in the standard recycling scenario due to its large Roche-lobe radius (>> the radius of the G-type main-sequence star). It is proposed here that this candidate redback millisecond pulsar binary could be created via accretion-induced collapse of an oxygen-neon-magnesium white dwarf.
学科主题天文学
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词ACCRETION-INDUCED COLLAPSE ; MILLISECOND PULSARS ; OPTICAL COUNTERPARTS ; MODEL ATMOSPHERES ; MESA ISOCHRONES ; NEUTRON-STAR ; TIME-SERIES ; BINARY ; EVOLUTION ; DISCOVERY
资助项目National SKA Program of China; Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST); National Development and Reform Commission; Chinese Academy of Sciences; NASA Explorer Program; Association of Universities for Research in Astronomy, Inc., under NASA[NAS 5-26555]; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0550300]; National Key R&D Program of China[2021YFA1600403]; CAS light of West China Program;[2020SKA0120100]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP Publishing Ltd
WOS记录号WOS:001135885000001
资助机构National SKA Program of China ; Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; National Development and Reform Commission ; Chinese Academy of Sciences ; NASA Explorer Program ; Association of Universities for Research in Astronomy, Inc., under NASA[NAS 5-26555] ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0550300] ; National Key R&D Program of China[2021YFA1600403] ; CAS light of West China Program ; [2020SKA0120100]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/26488]  
专题云南天文台_大样本恒星演化研究组
作者单位1.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China;
2.State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, People's Republic of China; j.lin@pku.edu.cn;
3.Department of Astronomy, School of Physics, Peking University, Beijing 100871, People's Republic of China; r.x.xu@pku.edu.cn;
4.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China;
5.National Astronomical Observatory, Chinse Academy of Sciences, Beijing 100101, People's Republic of China
6.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China;
推荐引用方式
GB/T 7714
Lin, Jie,Chen HL,Wang, Bojun,et al. 4FGL J1318.2+6754: A Long Orbital-period Redback Candidate[J]. ASTROPHYSICAL JOURNAL LETTERS,2024,960(1).
APA Lin, Jie,陈海亮,Wang, Bojun,&Xu, Renxin.(2024).4FGL J1318.2+6754: A Long Orbital-period Redback Candidate.ASTROPHYSICAL JOURNAL LETTERS,960(1).
MLA Lin, Jie,et al."4FGL J1318.2+6754: A Long Orbital-period Redback Candidate".ASTROPHYSICAL JOURNAL LETTERS 960.1(2024).

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来源:云南天文台

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