Hydrodynamical Models of Pulsar wind Bow-Shock Nebulae
| dc.creator | Bucciantini, N. | |
| dc.date | 2001-12-03 | |
| dc.date.accessioned | 2026-07-07T02:01:38Z | |
| dc.date.available | 2026-07-07T02:01:38Z | |
| dc.description | 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. | |
| dc.description | 4 pages, Latex, 3 Encapsulated PostScript figures "To appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P.O.Slane and B.M.Gaensler" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0112024 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0112024 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3822 | |
| dc.subject | Astrophysics | |
| dc.title | Hydrodynamical Models of Pulsar wind Bow-Shock Nebulae | |
| dc.type | text |