中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A discussion on the mass loss formulae for OH/IR stars

文献类型:期刊论文

作者Xiong GZ(熊关柱); Chen PS(陈培生)
刊名CHINESE ASTRONOMY AND ASTROPHYSICS
出版日期2000-10
卷号24期号:4页码:501-510
关键词OH/IR stars mass loss rate gas/dust ratio
ISSN号0275-1062
产权排序第一完成单位
通讯作者Xiong, GZ
英文摘要It is found that the mass loss rate derived from S-25/S-12 is generally greater;than that from the OH flux. This suggests an increasing loss rate with time. It is found that the gas-to-dust ratio decreases during the evolution Of OH/IR stars. An empirical relation between the gas-to-dust ratio and the dust mass loss rate is derived, leading to a formula for calculating the total mass loss rate directly from the IRAS 60 mum flux. OH/IR stars with silicate emission have a larger range of mass loss ratio, from 10(-7) to 10(-5) M-circle dot/yr; those with silicate absorption, a smaller range between 10(-5) and 10(-4) M-circle dot/yr. So a large increase in the mass loss rate takes place during the emission phase.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]RICH AGB STARS ; OH IR STARS ; LOSS RATES ; RED GIANTS ; EVOLUTION ; ENVELOPES ; SPECTRA
收录类别SCI
原文出处http://www.sciencedirect.com/science/article/pii/S0275106200000813
语种英语
WOS记录号WOS:000165799700012
源URL[http://ir.ynao.ac.cn/handle/114a53/3995]  
专题云南天文台_其他
作者单位Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 China
推荐引用方式
GB/T 7714
Xiong GZ,Chen PS. A discussion on the mass loss formulae for OH/IR stars[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2000,24(4):501-510.
APA Xiong GZ,&Chen PS.(2000).A discussion on the mass loss formulae for OH/IR stars.CHINESE ASTRONOMY AND ASTROPHYSICS,24(4),501-510.
MLA Xiong GZ,et al."A discussion on the mass loss formulae for OH/IR stars".CHINESE ASTRONOMY AND ASTROPHYSICS 24.4(2000):501-510.

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来源:云南天文台

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