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Searching for White Dwarf Candidates Formed Through Binary Evolution in Star Clusters

文献类型:期刊论文

作者Yan, Huahui11,12; Wang, Li11,12; Miller, David R.10; He, Chenyu11,12; Lin, Jiamao11,12; Pang, Xiaoying8,9; Zhao, Jingkun7; Guo, Jincheng6; Grijs, Richard de1,4,5; Ge HW(葛宏伟)3,13
刊名ASTROPHYSICAL JOURNAL
出版日期2026-03-10
卷号999期号:2
ISSN号0004-637X
DOI10.3847/1538-4357/ae3f07
产权排序第11完成单位
文献子类Article
英文摘要White dwarfs (WDs), the evolutionary endpoints of most stars, can form through both single-star and binary channels. While single-star evolutionary models enable reliable WD age estimates, binary evolution introduces interactions that can accelerate WD formation and result in a variety of exotic WDs, which may exhibit strong magnetic fields, rapid rotation, or even serve as potential gravitational wave sources. Such systems offer valuable insights into magnetic field generation, angular momentum evolution, and compact object physics. Star clusters, with their approximately coeval populations, allow precise age determination of member WDs. If a WD's total age derived from single-star evolution exceeds that of its host cluster, it likely indicates a binary origin. In this study, we use Gaia 5D astrometry to identify 439 WD candidates in 117 open clusters, with 244 likely formed via binary evolution. We discuss the possibility of dynamical ejection for WDs meeting only 2D (proper motion space) membership criteria. Spectroscopic observations further reveal a subset with strong magnetic fields and rapid rotation, supporting their binary evolutionary origin.
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FINAL MASS RELATION ; ASYMPTOTIC GIANT BRANCH ; HIGHLY VARIABLE-STARS ; SPECTROSCOPIC IDENTIFICATION ; GALACTIC CLUSTERS ; STELLAR TRACKS ; GAIA DR2 ; SPECTRAL CLASSIFICATION ; COOLING SEQUENCE ; ELECTRON-CAPTURE
资助项目MOST divided by National Natural Science Foundation of China (NSFC)[12233013]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001704358800001
出版者IOP Publishing Ltd
资助机构MOST divided by National Natural Science Foundation of China (NSFC)[12233013]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/29028]  
专题云南天文台_大样本恒星演化研究组
通讯作者Li, Chengyuan
作者单位1.School of Mathematical and Physical Sciences, Macquarie University, Balaclava Road, Sydney NSW 2109, Australia;
2.Instituto de Física y Astronomía, Universidad de Valparaíso, Avenida Gran Bretaña, 1111, Casilla 5030, Valparaíso, Chile
3.International Centre of Supernovae (ICESUN), Yunnan Key Laboratory of Supernova Research, Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming 650216, People’s Republic of China;
4.International Space Science Institute–Beijing, 1 Nanertiao, Zhongguancun, Hai Dian District, Beijing 100190, People’s Republic of China;
5.Astrophysics and Space Technologies Research Centre, Macquarie University, Balaclava Road, Sydney, NSW 2109, Australia;
6.Department of Scientific Research, Beijing Planetarium, Xizhimenwai Street, Beijing 100044, People’s Republic of China;
7.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China;
8.Shanghai Key Laboratory for Astrophysics, Shanghai Normal University, 100 Guilin Road, Shanghai 200234, People’s Republic of China;
9.Department of Physics, Xi’an Jiaotong—Liverpool University, 111 Ren’ai Road, Dushu Lake Science and Education Innovation District, Suzhou 215123, Jiangsu Province, People’s Republic of China;
10.Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1, Canada;
推荐引用方式
GB/T 7714
Yan, Huahui,Wang, Li,Miller, David R.,et al. Searching for White Dwarf Candidates Formed Through Binary Evolution in Star Clusters[J]. ASTROPHYSICAL JOURNAL,2026,999(2).
APA Yan, Huahui.,Wang, Li.,Miller, David R..,He, Chenyu.,Lin, Jiamao.,...&Li, Chengyuan.(2026).Searching for White Dwarf Candidates Formed Through Binary Evolution in Star Clusters.ASTROPHYSICAL JOURNAL,999(2).
MLA Yan, Huahui,et al."Searching for White Dwarf Candidates Formed Through Binary Evolution in Star Clusters".ASTROPHYSICAL JOURNAL 999.2(2026).

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