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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.
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页码:L29 / L33
页数:5
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