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Hydrodynamical Models of Pulsar wind Bow-Shock Nebulae | N. Bucciantini
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3 Dec 2001 | Subject: | astro-ph | Affiliation: | Dip. Astrofisica Univ. Firenze | Abstract: | 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. | Source: | arXiv, astro-ph/0112024 | Services: | Forum | Review | PDF | Favorites |
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