English

The CV period gap: still there

Astrophysics 2007-05-23 v1

Abstract

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.

Cite

@article{arxiv.astro-ph/9806007,
  title  = {The CV period gap: still there},
  author = {U. Kolb and A. R. King and H. Ritter},
  journal= {arXiv preprint arXiv:astro-ph/9806007},
  year   = {2007}
}

Comments

5 pages, incl. 4 figures. Accepted for publication in MNRAS

R2 v1 2026-07-22T09:40:20.825Z