Identification of new silicate carbon stars | |
Chen PS(陈培生)1,2; Dan HG(单红光)1,2 | |
刊名 | ASTROPHYSICS AND SPACE SCIENCE |
2011-10 | |
卷号 | 335期号:2页码:457-467 |
关键词 | Star: carbon star Star: infrared Infrared: spectrum |
ISSN号 | 0004-640X |
通讯作者 | Chen, PS (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. |
产权排序 | 第一完成单位 |
英文摘要 | 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. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | 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 |
收录类别 | SCI |
原文出处 | http://link.springer.com/article/10.1007%2Fs10509-011-0631-z |
语种 | 英语 |
WOS记录号 | WOS:000294680300016 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/4240] |
专题 | 云南天文台_其他 云南天文台_中国科学院天体结构与演化重点实验室 |
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 |
推荐引用方式 GB/T 7714 | Chen PS,Dan HG. Identification of new silicate carbon stars[J]. ASTROPHYSICS AND SPACE SCIENCE,2011,335(2):457-467. |
APA | Chen PS,&Dan HG.(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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