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The spectrum analysis of three chromospherically active binary stars
Gu SH(顾盛宏); Tan HS(谭徽松); Liu XF(刘学富)
Source Publication云南天文台台刊
1999
IssueS1Pages:361-371
ClassificationP152
Contribution Rank第1完成单位
Indexed By其他
AbstractThe authors present the research results on new CCD spectroscopic observations of three chromospherically active binary stars (BY Dra class), which were obtained by means of Coudé echelle spectrograph fed by the 2.16 m telescope at Beijing Astronomical Observatory. With the aid of stellar model atmosphere, the autors have analyzed these spectra and derived the average metal abundance and Li abundance of three systems. Using two special spectral lines, they have alsop discussed the chromospheric activity indicators of them.
Language英语
Subject Area天文学
Subtype期刊论文
ISSN1001-7526
Archive Date2002-10-16
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6765
Collection恒星物理研究组
Recommended Citation
GB/T 7714
Gu SH,Tan HS,Liu XF. The spectrum analysis of three chromospherically active binary stars[J]. 云南天文台台刊,1999(S1):361-371.
APA 顾盛宏,谭徽松,&刘学富.(1999).The spectrum analysis of three chromospherically active binary stars.云南天文台台刊(S1),361-371.
MLA 顾盛宏,et al."The spectrum analysis of three chromospherically active binary stars".云南天文台台刊 .S1(1999):361-371.
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