中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A Compact Object with a K-type Star Companion in the Solar Neighborhood: A Wide Postcommon Envelope Binary with a White Dwarf Candidate

文献类型:期刊论文

作者Lin, Jie2; Chen HL(陈海亮)1,6; Wang, Bojun5; Luo, Yudong4; Tang, Wenshi2; Huang, Bo3
刊名ASTROPHYSICAL JOURNAL
出版日期2026-02-20
卷号998期号:2
ISSN号0004-637X
DOI10.3847/1538-4357/ae3c77
产权排序第2完成单位
文献子类Article
英文摘要Post-common envelope binaries (PCEBs) consisting of a white dwarf (WD) plus a main-sequence star can constrain current prescriptions of common envelope evolution (CEE) and calibrate theoretical models of binary formation and evolution. Most PCEBs studied to date have typical orbital periods of hours to a few days and can be well explained by assuming inefficient CEE to expel the envelope. However, there are currently several systems with relatively wide orbital periods (>18 days). To explain these wide PCEBs, additional sources of energy have been suggested to be taken into account. Here, we present the discovery and observational characterization of a compact object (M >= 0.58 M-circle dot) with a K-type star companion in the solar neighborhood (d similar to 112 pc) and an orbital period of P-orb similar to 14 days. The compact object binary is likely to be a system consisting of a WD and a barium dwarf, making it the shortest-period barium star binary candidate known. Such a system with an orbital period within the gap between tight and wide binaries provides a test of whether additional energy sources are required to explain its formation. Using binary evolution models, we investigate the evolutionary history of this wide PCEB system and find that the observed properties of this source can be explained without invoking any extra energy source.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地No.2 The Distillery, Glassfields, Avon Street, Bristol, ENGLAND
WOS关键词STELLAR ATMOSPHERIC PARAMETERS ; NEUTRON-STAR ; DATA RELEASE ; CONVECTIVE BOUNDARIES ; PATHWAYS SURVEY ; FGK STARS ; EVOLUTION ; LAMOST ; MODULES ; GAIA
资助项目National Natural Science Foundation of China[12403055]; National Natural Science Foundation of China[12221003]; National Natural Science Foundation of China[12335009]; National Natural Science Foundation of China[12288102]; National Natural Science Foundation of China[12333008 and 12422305]; Postdoctoral Fellowship Program of CPSF[GZC20240905]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001696145100001
出版者IOP Publishing Ltd
资助机构National Natural Science Foundation of China[12403055, 12221003, 12335009, 12288102, 12333008 and 12422305] ; Postdoctoral Fellowship Program of CPSF[GZC20240905]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28991]  
专题云南天文台_大样本恒星演化研究组
通讯作者Lin, Jie
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People’s Republic of China;
2.Department of Astronomy, Xiamen University, Xiamen, Fujian 361005, People’s Republic of China; j.lin@pku.edu.cn;
3.Institut de Ciències de l’Espai (ICE-CSIC), Campus UAB, Can Magrans S/N, E-08193 Cerdanyola del Vallès, Catalonia, Spain
4.School of Physics, Peking University, and Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People’s Republic of China;
5.National Astronomical Observatory, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China;
6.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People’s Republic of China;
推荐引用方式
GB/T 7714
Lin, Jie,Chen HL,Wang, Bojun,et al. A Compact Object with a K-type Star Companion in the Solar Neighborhood: A Wide Postcommon Envelope Binary with a White Dwarf Candidate[J]. ASTROPHYSICAL JOURNAL,2026,998(2).
APA Lin, Jie,陈海亮,Wang, Bojun,Luo, Yudong,Tang, Wenshi,&Huang, Bo.(2026).A Compact Object with a K-type Star Companion in the Solar Neighborhood: A Wide Postcommon Envelope Binary with a White Dwarf Candidate.ASTROPHYSICAL JOURNAL,998(2).
MLA Lin, Jie,et al."A Compact Object with a K-type Star Companion in the Solar Neighborhood: A Wide Postcommon Envelope Binary with a White Dwarf Candidate".ASTROPHYSICAL JOURNAL 998.2(2026).

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