Modelling the equatorial activity in SS433

被引：0
作者：
Smponias, T.
机构：
来源：
Recent Advances in Astronomy and Astrophysics | 2006年 / 848卷
关键词：
binaries : eclipsing; stars : winds; outflows; plasmas; radiation mechanisms : thermal; binaries : close; radio continuum : stars; stars : individual (SS433);
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The jets in SS433 were modelled using a two-dimensional classical hydrocode and a dynamical mechanism was suggested to explain the observed equatorial radio features in SS433. The modelling provided constraints to a number of jet and stellar wind parameters for the jet-wind system. An ambient density falling off away from the jet base was found to offer the best results for enhancing the equatorial region activity.
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页码：442 / 446
页数：5
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