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IRAS 17213-3841: A late-type carbon-rich star or an early-type emission-line star?
Chen PS(陈培生)1; Zhang P(张品)1,2; Chen, PS (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, Kunming 650011, Peoples R China.
发表期刊CHINESE ASTRONOMY AND ASTROPHYSICS
2004-04
卷号28期号:2页码:160-165
DOI10.1016/j.chinastron.2004.04.006
产权排序第1完成单位
收录类别SCI
关键词Star : Carbon Star : Early-type Star : Emission Line Infrared : Star
摘要IRAS 17213-3841 is listed in a new edition of the Catalogue of Carbon Stars as a, carbon-rich star. However, the IRAS low-resolution spectrum of the star shows the oxygen-rich silicate emission feature. Spectral observations show that the star is an early-type emission-line star near the zero age main sequence with spectral type O9/B0, and is not a carbon star. Therefore it should be removed from the catalogue of carbon stars. The near infrared-IRAS two-colour diagram method used to identify IRAS 17213-3841 as a carbon star is not completely reliable and care should be exercised when using it for identification of carbon stars.
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:000222026000005
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]NEAR-INFRARED PHOTOMETRY ; LOW-RESOLUTION SPECTRA ; POINT-SOURCE CATALOG ; SPACE DISTRIBUTION ; IR PHOTOMETRY ; IDENTIFICATIONS ; CLASSIFICATION ; ENVELOPES ; SAMPLE ; GALAXY
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被引频次:3[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/114a53/4179
专题其他
通讯作者Chen, PS (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, Kunming 650011, Peoples R China.
作者单位1.Yunnan Observatory, P.O.Box 110, Kunming, Yunnan 650011, People's Republic of China
2.Cosmic Ray Institute, Yunnan University, Kunming 650091 P.R. China
第一作者单位中国科学院云南天文台
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Chen PS,Zhang P,Chen, PS . IRAS 17213-3841: A late-type carbon-rich star or an early-type emission-line star?[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2004,28(2):160-165.
APA Chen PS,Zhang P,&Chen, PS .(2004).IRAS 17213-3841: A late-type carbon-rich star or an early-type emission-line star?.CHINESE ASTRONOMY AND ASTROPHYSICS,28(2),160-165.
MLA Chen PS,et al."IRAS 17213-3841: A late-type carbon-rich star or an early-type emission-line star?".CHINESE ASTRONOMY AND ASTROPHYSICS 28.2(2004):160-165.
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