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CARBON STARS WITH INFRARED SPECTRA IN GROUP P OF THE IRAS/LRS DATABASE
Chen PS(陈培生)1; Yang, XH2
刊名ASTRONOMICAL JOURNAL
2012-10
卷号144期号:4页码:104-107
关键词infrared: stars stars: AGB and post-AGB stars: carbon
ISSN号0004-6256
通讯作者Chen, PS (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China.
产权排序第一完成单位
英文摘要Sources with infrared spectra in Group P of the IRAS/LRS database all show polycyclic aromatic hydrocarbon features. They are often planetary nebulae, H II regions, reflection/dark nebulae, Wolf-Rayet stars, or external galaxies. However, we noted that some carbon stars are also included in this group. We searched for and investigated all infrared spectra in Group P of the IRAS/LRS database. Finally, we found 11 previously known carbon stars and identified 8 new candidate carbon stars in Group P. Infrared spectra of these stars may present the 11.2 mu m SiC emission features indicative of their carbon-rich 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]OBJECTIVE-PRISM PLATES ; IDENTIFICATION ; PHOTOMETRY ; EMISSION ; CATALOG
收录类别SCI
原文出处http://iopscience.iop.org/article/10.1088/0004-6256/144/4/104/meta
语种英语
WOS记录号WOS:000308919300014
内容类型期刊论文
源URL[http://ir.ynao.ac.cn/handle/114a53/4243]  
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 and Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
2.Department of Physics, Chongqing University, Chongqing 400044, China
推荐引用方式
GB/T 7714
Chen PS,Yang, XH. CARBON STARS WITH INFRARED SPECTRA IN GROUP P OF THE IRAS/LRS DATABASE[J]. ASTRONOMICAL JOURNAL,2012,144(4):104-107.
APA Chen PS,&Yang, XH.(2012).CARBON STARS WITH INFRARED SPECTRA IN GROUP P OF THE IRAS/LRS DATABASE.ASTRONOMICAL JOURNAL,144(4),104-107.
MLA Chen PS,et al."CARBON STARS WITH INFRARED SPECTRA IN GROUP P OF THE IRAS/LRS DATABASE".ASTRONOMICAL JOURNAL 144.4(2012):104-107.
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