The cataclysmic variable period gap: still there

被引:36
|
作者
Kolb, U [1 ]
King, AR
Ritter, H
机构
[1] Univ Leicester, Astron Grp, Leicester LE1 7RH, Leics, England
[2] Max Planck Inst Astrophys, D-85740 Garching, Germany
关键词
accretion; accretion discs; binaries : close; stars : evolution; stars : low-mass; novae; cataclysmic variables;
D O I
10.1046/j.1365-8711.1998.01854.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider a recently proposed alternative explanation of the CV period gap in terms of a revised mass-radius relation for the lower main sequence. We show that no such thermal equilibrium relation is likely to produce a true gap. Using population synthesis techniques we calculate a model population that obeys the claimed equilibrium mass-radius relation. A theoretical period histogram obtained from this population shows two prominent period spikes rather than a gap. We consider also recent arguments suggesting that the period gap itself may not be real. We argue that, far from demonstrating a weakness of the interrupted braking picture, the fact that most CV subtypes prefer one side of the gap or the other is actually an expected consequence of this model.
引用
收藏
页码:L29 / L33
页数:5
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