Wolf-Rayet stars, binaries, black holes

被引：0
|
作者：
Van der Hucht, KA [1 ]
机构：
[1] Space Res Org Netherlands, NL-3584 CA Utrecht, Netherlands
来源：
EVOLUTION OF THE MILKY WAY: STARS VERSUS CLUSTERS | 2000年 / 255卷
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We review the literature of the past two decades on the possible evolution from the massive star Wolf-Rayet phase to the black hole phase, and on the masses of WR stars observed in binary systems. A list of 55 WR binaries is presented. The 19 WR binaries with RV solutions have WN star masses in the range 2-55 M. and WC star masses in the range 9-16 M.. We discuss four candidate WR+BH systems: WR 145a (Cyg X-3), WR 148 (HD 197406), BAT99-102 (R 140a2), and BAT99-116 (Mk 34).
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页码：125 / 138
页数：14
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