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Measurement of the metal abundance and magnetic field of the late-type stars HR 5553, epsilon Eri and 70 Oph
Liu, XF1,4; Zhao, G2,4; Qiu, HM1,2,4; Dan HG(单红光)3,4
发表期刊CHINESE ASTRONOMY AND ASTROPHYSICS
1999-07
卷号23期号:3页码:361-370
DOI10.1016/S0275-1062(99)00066-1
产权排序第3完成单位
收录类别SCI
关键词Late-type Active Star Metal Abundance Magnetic Field
摘要This paper presents high-resolution (6x10(4)), high S/N (200-500) spectra of three K-type chromospheric active stars, HR 5553, epsilon Eri and 70 Oph. The observations were made using an echelle spectrograph on the 2.16-m telescope of Beijing/Xinglong Station in 1995 and 1996. The atmosphere parameters and the abundances of 13 metals for these stars were determined from a detailed spectroscopic analysis and their magnetic field strength B and filling factor ct found by the Stenflo-Lindegren method.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0275-1062
URL查看原文
WOS记录号WOS:000082410600014
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]CA-II-H ; BINARY STARS ; K-DWARFS ; ERIDANI ; SOLAR ; LINES ; CHROMOSPHERES ; SINGLE
引用统计
被引频次:2[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5146
专题恒星物理研究组
通讯作者Liu, XF
作者单位1.Department of Astronomy, Beijing Normal University, Beijing 100875 China
2.Department of Astronomy, Beijing Normal University, Beijing 100875 China
3.Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 China
4.Joint Laboratory for Optical Astronomy, Chinese Academy of Sciences, Beijing 100080 China
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GB/T 7714
Liu, XF,Zhao, G,Qiu, HM,et al. Measurement of the metal abundance and magnetic field of the late-type stars HR 5553, epsilon Eri and 70 Oph[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,1999,23(3):361-370.
APA Liu, XF,Zhao, G,Qiu, HM,&Dan HG.(1999).Measurement of the metal abundance and magnetic field of the late-type stars HR 5553, epsilon Eri and 70 Oph.CHINESE ASTRONOMY AND ASTROPHYSICS,23(3),361-370.
MLA Liu, XF,et al."Measurement of the metal abundance and magnetic field of the late-type stars HR 5553, epsilon Eri and 70 Oph".CHINESE ASTRONOMY AND ASTROPHYSICS 23.3(1999):361-370.
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