首页 | 本学科首页   官方微博 | 高级检索  
     


Three-dimensional numerical simulation of gaseous flow structure in semidetached binaries
Authors:D. V. Bisikalo,A. A. Boyarchuk,V. M. Chechetkin,O. A. Kuznetsov,&   D. Molteni
Affiliation:Institute of Astronomy of Russian Academy of Sciences, 48 Pyatnitskaya str., Moscow 109017, Russia,;Keldysh Institute of Applied Mathematics, 4 Miusskaya sq., Moscow 125047, Russia,;Dipartimento di Scienze Fisiche ed Astronomiche, Universitàdi Palermo, 36 Via Archirafi, I-90123 Palermo, Italy
Abstract:
Keywords:accretion    accretion discs    hydrodynamics    methods: numerical    binaries: close    stars: mass-loss
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号