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Analysis of high-resolution spectra of mildly metal-poor stars I. Spectral data and equivalent widths
Zhong, HY; Zhao, G; Qiu, HM
2002-10-01
Source PublicationCHINESE ASTRONOMY AND ASTROPHYSICS
Volume26Issue:4Pages:424-431
AbstractA number of high resolution and high signal-to-noise ratio spectra of mildly metal-poor stars were obtained with the coude echelle spectrograph attached to the 2.16 m telescope at Xinglong Observation Base of Beijing Astronomical Observatory. The spectra of seven mildly metal-poor stars were processed with the MIDAS software package, and the equivalent widths of their spectral lines were measured. The measured equivalent widths together with an error analysis are presented.
KeywordStar : abundanceStar Star : Evolution Line : Profile
Indexed BySCI
Language英语
WOS IDWOS:000180030600006
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8492
Collection光学天文研究部
AffiliationChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Zhong, HY,Zhao, G,Qiu, HM. Analysis of high-resolution spectra of mildly metal-poor stars I. Spectral data and equivalent widths[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2002,26(4):424-431.
APA Zhong, HY,Zhao, G,&Qiu, HM.(2002).Analysis of high-resolution spectra of mildly metal-poor stars I. Spectral data and equivalent widths.CHINESE ASTRONOMY AND ASTROPHYSICS,26(4),424-431.
MLA Zhong, HY,et al."Analysis of high-resolution spectra of mildly metal-poor stars I. Spectral data and equivalent widths".CHINESE ASTRONOMY AND ASTROPHYSICS 26.4(2002):424-431.
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