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Identification of new silicate carbon stars
Chen PS(陈培生)1,2; Dan HG(单红光)1,2; Chen, PS (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊ASTROPHYSICS AND SPACE SCIENCE
2011-10
卷号335期号:2页码:457-467
DOI10.1007/s10509-011-0631-z
产权排序第1完成单位
收录类别SCI
关键词Star: Carbon Star Star: Infrared Infrared: Spectrum
摘要IRAS low-resolution spectra for 17 sources are presented in this paper. Together with the carbon star catalog, information from recent literatures, the ISO observation and the IRAS two-color diagram, it is found that among them 5 sources are new silicate carbon stars, 5 sources are candidates of silicate carbon stars and other 7 sources are probable candidates of silicate carbon stars. Some discussions are made for their infrared properties.
项目资助者NNSFC [10503011, 10533050] ; Chinese Academy of Sciences
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-640X
URL查看原文
归档日期2011-10-17
WOS记录号WOS:000294680300016
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]RICH CIRCUMSTELLAR ENVELOPES ; LOW-RESOLUTION SPECTRA ; FLUX-LIMITED SAMPLE ; NORTHERN MILKY-WAY ; LOSING AGB STARS ; SIO MASER SURVEY ; IRAS SOURCES ; EU-ANDROMEDAE ; DUST FEATURES ; BM GEMINORUM
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被引频次:5[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/114a53/4240
专题其他
中国科学院天体结构与演化重点实验室
通讯作者Chen, PS (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
作者单位1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 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,Dan HG,Chen, PS . Identification of new silicate carbon stars[J]. ASTROPHYSICS AND SPACE SCIENCE,2011,335(2):457-467.
APA Chen PS,Dan HG,&Chen, PS .(2011).Identification of new silicate carbon stars.ASTROPHYSICS AND SPACE SCIENCE,335(2),457-467.
MLA Chen PS,et al."Identification of new silicate carbon stars".ASTROPHYSICS AND SPACE SCIENCE 335.2(2011):457-467.
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