Gas flow in close binary star systems
Astrophysics
2007-05-23 v1
Abstract
We first present a summary of our numerical work on accretion discs in close binary systems. Our recent studies on numerical simulations of the surface flow on the mass-losing star in a close binary star is then reviewed.
Cite
@article{arxiv.astro-ph/0402146,
title = {Gas flow in close binary star systems},
author = {K. Oka and T. Matsuda and I. Hachisu and H. Boffin},
journal= {arXiv preprint arXiv:astro-ph/0402146},
year = {2007}
}
Comments
8 pages, 5 figures, to appear in the proceedings of 6th International Nobeyama Workshop