Gas flow in close binary star systems

被引：1

作者：

Matsuda, T ^{[1
]}

Oka, K ^{[1
]}

Hachisu, I ^{[1
]}

Boffin, HMJ ^{[1
]}

机构：

[1] Kobe Univ, Dept Earth & Planetary Sci, Kobe, Hyogo 6578501, Japan

来源：

New Developments in Computational Fluid Dynamics | 2005年 / 90卷

关键词：

D O I：

10.1007/3-540-31261-7_18

中图分类号：

O3 [力学];

学科分类号：

08 ; 0801 ;

摘要：

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.

引用

页码：198 / 205

页数：8

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