THE POSSIBILITY OF NON-SYNCHRONISM OF CONVECTIVE SECONDARIES IN CLOSE BINARY STARS

被引：46

作者：

CAMPBELL, CG ^{[1
]}

PAPALOIZOU, J ^{[1
]}

机构：

[1] UNIV LONDON QUEEN MARY COLL,DEPT APPL MATH,LONDON E1 4NS,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1983年 / 204卷 / 02期

关键词：

Binary star - Binary systems - Low-mass - Synchronization time - Synchronous velocity - Turbulent viscosity - Velocity field;

D O I：

10.1093/mnras/204.2.433

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

收藏

页码：433 / 447

页数：15

相关论文

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