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

关键词：

D O I：

暂无

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).

引用

页码：125 / 138

页数：14

共 50 条

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