Binary post-AGB stars: Protosymbiotic systems?

被引：0
|
作者：
Van Winckel, H [1 ]
机构：
[1] Katholieke Univ Leuven, Inst Sterrenkunde, B-3001 Heverlee, Belgium
来源：
SYMBIOTIC STARS PROBING STELLAR EVOLUTION | 2003年 / 303卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The binary nature of symbiotic stars, consisting of a hot compact component and a mass-losing giant, is beyond discussion. In this contribution we discuss possible precursors and focus on the binaries in a post-AGB stage of evolution in which the system consists of a strongly evolved post-AGB object and a mostly unseen and unevolved companion. We list the most important characteristics of these systems and discuss the possible evolutionary connection with symbiotic binaries.
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页码：294 / 297
页数：4
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