Gas flow in close binary star systems

2004/02/06 by K. Oka, Kazutaka Oka, T. Matsuda +9
Engineering · Physics and Astronomy · #Astro and Planetary Science #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Phase Equilibria and Thermodynamics #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0402146

8 pages, 5 figures, to appear in the proceedings of 6th International Nobeyama Workshop

arxiv created 2004/02/06 · openalex publication_date 2004/02/06 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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.

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