类灾变星轨道周期分布之探讨
天体物理学
2009-10-30 v1
摘要
Using the latest compilation of cataclysmic variable orbital periods by Ritter & Kolb we argue against Verbunt's conclusion that the period gap is not significant for nova-like variables. We also discuss the relation of the VY Scl stars to the dwarf novae.
引用
@article{arxiv.astro-ph/9802041,
title = {On the orbital period distribution of cataclysmic variables},
author = {Coel Hellier and T. Naylor},
journal= {arXiv preprint arXiv:astro-ph/9802041},
year = {2009}
}
备注
3 pages, 3 figures, LaTeX, To appear in MNRAS. Also at http://www.astro.keele.ac.uk/~ch/