The implications of disc instabilities on cataclysmic variable structure and evolution
天体物理学
2007-05-23 v1
摘要
Applications of the thermal-viscous disc instability model to various classes of cataclysmic variable very often require the accretion disc to be truncated. I argue that in most cases this inner truncation must be due to the white dwarf's magnetic field.
关键词
引用
@article{arxiv.astro-ph/0402190,
title = {The implications of disc instabilities on cataclysmic variable structure and evolution},
author = {J. -P. Lasota},
journal= {arXiv preprint arXiv:astro-ph/0402190},
year = {2007}
}
备注
To appear in: Compact Binaries in the Galaxy and Beyond, IAU Coll. 194, editors E. Sion and G. Tovmassian