Hydrodynamical models of pulsar wind bow-shock nebulae

被引：0
|
作者：
Bucciantini, N [1 ]
机构：
[1] Univ Florence, Dipartimento Astron & Sci Spazio, I-50121 Florence, Italy
来源：
NEUTRON STARS IN SUPERNOVA REMNANTS | 2002年 / 271卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present hydrodynamical simulations, using a 2-D two fluid model, of bow shocks in a representative regime for pulsar wind driven bow-shock nebulae. We also investigate the behaviour of a passive toroidal magnetic field wounded around the pulsar velocity direction. Moreover we estimate the opacity of the bow-shock to penetration of ISM neutral hydrogen. Finally we compare these numerical results with those from an analytical model.
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页码：109 / 112
页数：4
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