WHITE-DWARF ROTATIONAL EQUILIBRIA IN MAGNETIC CATACLYSMIC VARIABLE-STARS

被引：58

作者：

WARNER, B ^{[1
]}

WICKRAMASINGHE, DT ^{[1
]}

机构：

[1] AUSTRALIAN NATL UNIV,DEPT MATH,CANBERRA,ACT 2600,AUSTRALIA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1991年 / 248卷 / 03期

关键词：

D O I：

10.1093/mnras/248.3.370

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The magnetic cataclysmic variable stars (polars, intermediate polars and DQ Her stars) are grouped about three lines in the orbital period-spin period diagram. This segregation is shown to be the consequence of competition between braking and accretion torques when combined with the effects of cyclical variations in rate of mass transfer.

引用

页码：370 / 376

页数：7

共 29 条

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