中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A New Catalog of Am-type Chemically Peculiar Stars Based on LAMOST

文献类型:期刊论文

作者Zhang, Xianfei2,3; Jeffery, C. Simon6; Su J(苏杰)1,4,5; Bi, Shaolan2,3
刊名ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
出版日期2023-05-01
卷号266期号:1
ISSN号0067-0049
DOI10.3847/1538-4365/acc4b5
产权排序第4完成单位
文献子类Article
英文摘要A total of about 21,600 Am candidates were detected with the MKCLASS code based on the low-resolution spectra of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope Data Releases 8 (v1.0), 9 (v0), and 10 (v0), which greatly expands the database of Am-type stars. By crossmatching the known catalogs of Am stars and our Am candidates with the AAVSO International Variable Star Index catalog, a catalog of the largest eclipsing Am binaries was obtained, which includes 754 binaries and provides a substantial sample with which to study Am stars. Fundamental information, including atmospheric parameters of the two kinds of candidates, are collected and listed in the catalogs, such as temperature, log g, and metallicity. We further carried out statistical analysis of the types of parameters. In our new catalog, there are some Am candidates with a temperature lower than 7000 K and some eclipsing Am binary candidates with a period of less than 1 day, which poses challenges to the slow rotation of stars classified as type Am observed in previous research. These candidates are significant and provide a great opportunity to explore the real relationship between Am-type stars' peculiarity and slow stellar rotation. The Hertzsprung-Russell diagram of Am stars and the primary stars of eclipsing Am binary candidates indicate that a majority of the Am stars and almost all primary stars of binaries are in or around the main-sequence evolution stage.
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METAL ABUNDANCES ; BINARY-SYSTEMS ; RELEASE ; ROTATION ; AP ; CLASSIFICATION ; STABILIZATION ; PARAMETERS ; SPECTRA ; MEMBERS
资助项目Chinese National Natural Science Foundation of China[12103030]; Chinese National Natural Science Foundation of China[11922306]; Natural Science of Shandong Province[ZR2020QA048]; Natural Science of Shandong Province[ZR2021QA082]; Natural Science Foundation of Xinjiang Uygur Autonomous Rejion[2022DO1A164]; National Science Foundation of China (NSFC)[U1831109]; Chinese Academy of Sciences (CAS)[U1831109]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001138816400001
出版者IOP Publishing Ltd
资助机构Chinese National Natural Science Foundation of China[12103030, 11922306] ; Natural Science of Shandong Province[ZR2020QA048, ZR2021QA082] ; Natural Science Foundation of Xinjiang Uygur Autonomous Rejion[2022DO1A164] ; National Science Foundation of China (NSFC)[U1831109] ; Chinese Academy of Sciences (CAS)[U1831109]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/26475]  
专题云南天文台_恒星物理研究组
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.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China;
2.Institute for Frontier in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, People's Republic of China; zxf@bnu.edu.cn;
3.Department of Astronomy, Beijing Normal University, Beijing 100875, People's Republic of China;
4.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China
5.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, People's Republic of China;
6.Armagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, UK;
推荐引用方式
GB/T 7714
Zhang, Xianfei,Jeffery, C. Simon,Su J,et al. A New Catalog of Am-type Chemically Peculiar Stars Based on LAMOST[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2023,266(1).
APA Zhang, Xianfei,Jeffery, C. Simon,苏杰,&Bi, Shaolan.(2023).A New Catalog of Am-type Chemically Peculiar Stars Based on LAMOST.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,266(1).
MLA Zhang, Xianfei,et al."A New Catalog of Am-type Chemically Peculiar Stars Based on LAMOST".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 266.1(2023).

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来源:云南天文台

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