Probing the shape of the brown dwarf desert around main-sequence A-F-G-type stars using post-common-envelope WD-BD binaries
文献类型:期刊论文
作者 | Chen, Zhangliang4,5; Chen, Yizhi4,5; Chen, Chen4,5; Ge HW(葛宏伟)1,2,3![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2024-07-17 |
卷号 | 687 |
关键词 | binaries: close brown dwarfs white dwarfs |
ISSN号 | 0004-6361 |
DOI | 10.1051/0004-6361/202348870 |
产权排序 | 第3完成单位 |
文献子类 | Article |
英文摘要 | Context. Brown dwarfs (BDs) with masses in the range 40-60 M-Jup are rare around solar-type main-sequence (MS) stars, which gives rise to the brown dwarf desert (BDD). One caveat associated with previous studies of BDD is the relatively limited sample size of MS-BD binaries with accurately determined BD masses. Aims. We aim to produce a large sample of BD companions with precisely determined masses around MS A-F-G-type stars using observations of post-common-envelope white dwarf (WD)-BD binaries. Methods. We employed the rapid binary evolution code COMPAS to deduce the properties of MS-BD binary progenitors from post-common-envelope WD-BD binaries. With this method, we increase the sample of directly observed MS-BD binaries, enriching the data available for analyzing the BDD around MS A-F-G-type stars. Results. Our study opens a new window for studying the shape of the BDD around A-F-G-type MS stars in the short-period regime. We find tentative evidence, albeit with a small sample size, that the driest part of the BDD around A-F-G-type stars may extend into an orbital period of several hundred days. More post-common-envelope WD-BD binaries detected in the future will advance our understanding of the BDD around A-F-G-type stars. |
学科主题 | 天文学 ; 恒星与银河系 |
URL标识 | 查看原文 |
出版地 | 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE |
WOS关键词 | LOW-MASS COMPANIONS ; WHITE-DWARF ; TRANSITING EXOPLANETS ; SUBSTELLAR COMPANIONS ; STELLAR COMPANIONS ; SHORT-PERIOD ; EVOLUTION ; ORBIT ; SDSS ; PROJECT |
资助项目 | National Key R&D Program of China[2021YFA1600403]; National Key R&D Program of China[2020YFC2201400]; NSFC[12073092]; NSFC[12103097]; NSFC[12103098]; NSFC[12288102]; NSFC[12125303]; NSFC[12173081]; China Manned Space Project[CMS-CSST-2021-B09]; Key research program of frontier sciences, CAS[ZDBS-LY-7005]; Yunnan Fundamental Research Projects[202101AV070001] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:001271688200001 |
出版者 | EDP SCIENCES S A |
资助机构 | National Key R&D Program of China[2021YFA1600403, 2020YFC2201400] ; NSFC[12073092, 12103097, 12103098, 12288102, 12125303, 12173081] ; China Manned Space Project[CMS-CSST-2021-B09] ; Key research program of frontier sciences, CAS[ZDBS-LY-7005] ; Yunnan Fundamental Research Projects[202101AV070001] |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/27499] ![]() |
专题 | 云南天文台_大样本恒星演化研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
作者单位 | 1.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, PR China 2.Key Laboratory for Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, PO Box 110 Kunming 650216, PR China; 3.Yunnan Observatories, Chinese Academy of Sciences, 396 YangFangWang, Guandu District, Kunming 650216, PR China; 4.CSST Science Center for the Guangdong-HongKong-Macau Great Bay Area, Sun Yat-sen University, Zhuhai 519082, PR China; 5.School of Physics and Astronomy, Sun Yat-sen University, Zhuhai 519082, PR China; |
推荐引用方式 GB/T 7714 | Chen, Zhangliang,Chen, Yizhi,Chen, Chen,et al. Probing the shape of the brown dwarf desert around main-sequence A-F-G-type stars using post-common-envelope WD-BD binaries[J]. ASTRONOMY & ASTROPHYSICS,2024,687. |
APA | Chen, Zhangliang,Chen, Yizhi,Chen, Chen,葛宏伟,&Ma, Bo.(2024).Probing the shape of the brown dwarf desert around main-sequence A-F-G-type stars using post-common-envelope WD-BD binaries.ASTRONOMY & ASTROPHYSICS,687. |
MLA | Chen, Zhangliang,et al."Probing the shape of the brown dwarf desert around main-sequence A-F-G-type stars using post-common-envelope WD-BD binaries".ASTRONOMY & ASTROPHYSICS 687(2024). |
入库方式: OAI收割
来源:云南天文台
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