EVOLUTION OF MASSIVE CLOSE BINARIES

被引：0

作者：

DEGREVE, JP ^{[1
]}

DELOORE, C ^{[1
]}

机构：

[1] UNIV ANTWERP,ASTROPHYS RES GRP,RUCA,BELGIUM

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1992年 / 96卷 / 03期

关键词：

BINARIES; CLOSE; STARS; EVOLUTION; WOLF-RAYET;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

An analysis is given of the various aspects of massive close binary evolution, as derived from earlier presented calculations. Apart from the conditions at the beginning and the end of the mass transfer, we specially analyse the evolution covering the core helium burning phase of the primary. For stars with initial mass of the donor M1i greater-than-or-equal-to 20 M. this phase is identified with the WR phase. Finally, the systems at the end of core helium burning are evaluated as possible progenitor systems for the observed massive X ray sources.

引用

页码：653 / 663

页数：11

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