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Discussion on candidates for the M stars with 11.2 mu m SiC feature
Chen PS(陈培生); Gao YF(高亦菲); Dan HG(单红光); Wang XH(汪洵浩); Chen, PS (reprint author), CAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China.
发表期刊NEW ASTRONOMY
2004-01
卷号9期号:1页码:17-26
DOI10.1016/S1384-1076(03)00088-5
产权排序第1完成单位
收录类别SCI ; EI
关键词Stars : Late-type Stars : Chemically Peculiar Infrared : Stars
摘要The oxygen-rich stars with SiC emission features are unexpected according to the evolutionary theory in the late stage of stellar evolution. After the careful re-examination of such samples reported previously and searching for new samples, seven stars are found to be the candidates of the M stars with 11.2 mum SiC emission feature. However, with the IRAS low-resolution spectrum, the IRAS two colour diagram and other information, it is seen that no strong candidates for oxygen-rich AGB stars with carbon-rich circumstellar dust could be found so far. (C) 2003 Elsevier B.V. All rights reserved.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN1384-1092
URL查看原文
归档日期2003-11-17
WOS记录号WOS:000186681400002
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]LOW-RESOLUTION SPECTRA ; UNUSUAL DUST SHELLS ; CRYSTALLINE SILICATE DUST ; INFRARED CARBON STARS ; GIANT BRANCH STARS ; EVOLVED STARS ; SPACE DISTRIBUTION ; STELLAR EVOLUTION ; IRAS SPECTRA ; RED GIANTS
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被引频次:1[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/114a53/4184
专题其他
通讯作者Chen, PS (reprint author), CAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China.
作者单位National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China
第一作者单位中国科学院云南天文台
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Chen PS,Gao YF,Dan HG,et al. Discussion on candidates for the M stars with 11.2 mu m SiC feature[J]. NEW ASTRONOMY,2004,9(1):17-26.
APA Chen PS,Gao YF,Dan HG,Wang XH,&Chen, PS .(2004).Discussion on candidates for the M stars with 11.2 mu m SiC feature.NEW ASTRONOMY,9(1),17-26.
MLA Chen PS,et al."Discussion on candidates for the M stars with 11.2 mu m SiC feature".NEW ASTRONOMY 9.1(2004):17-26.
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