| Mira Symbiotic Stars |
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| 作者姓名： | Guo-Liang Lü |
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| 作者单位： | Guo-Liang L1，2，Chun-Hua Zhu2 and Zhan-Wen Han1 1 National Astronomical Observatories / Yunnan Observatory，Chinese Academy of Sciences，Kunming 650011; 2 Department of Physics，Xinjiang University，Urumqi 830046 |
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| 基金项目： | 国家自然科学基金;中国科学院基金;新疆大学校科研和教改项目 |
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| 摘 要： | 1 INTRODUCTION Symbiotic stars (SSs) are interacting binaries consisting of a cool giant, a hot compact companion and an H II region (Berman 1932; Boyarchuk 1967; Boyarchuk 1968). The cool component is a red giant (RG) that belongs either to the first gia…
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| 关 键 词： | binaries: symbiotic—Galaxy: stellar content—stars: Mira variables |
Mira Symbiotic Stars |
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| Chun-Hua Zhu,Zhan-Wen Han.Mira Symbiotic Stars[J].Chinese Journal of Astronomy and Astrophysics,2007,7(1):101-110. |
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| Authors: | Chun-Hua Zhu Zhan-Wen Han |
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| Institution: | [1]National Astronomical Observatories / Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 [2]Department of Physics, Xinjiang University, Urumqi 830046 |
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| Abstract: | |
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| Keywords: | binaries: symbiotic - Galaxy: stellar content - stars: Mira variables |
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