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)![]() ![]() |
刊名 | CHINESE ASTRONOMY AND ASTROPHYSICS
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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. |
入库方式: OAI收割
来源:云南天文台
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