posted on 2019-10-23, 15:56authored byU. Kolb, A. R. King, H. Ritter
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 it.
Funding
ARK thanks the U.K. Particle Physics
and Astronomy Research Council for a Senior Fellowship.
Theoretical astrophysics research at Leicester is supported
by a PPARC Rolling Grant.
History
Citation
Monthly Notices of the Royal Astronomical Society, 1998, 298 (2), pp. L29-L33
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Version
AM (Accepted Manuscript)
Published in
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press (OUP), Royal Astronomical Society