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A&A 387, 1066-1073 (2002)
DOI: 10.1051/0004-6361:20020495
Pulsar bow-shock nebulae
II. Hydrodynamical simulation
N. BucciantiniDip. di Astronomia e Scienza dello Spazio, Università di Firenze, Largo E.Fermi 5, 50125 Firenze, Italy
(Received 14 November 2001 / Accepted 19 March 2002 )
Abstract
We present hydrodynamical simulations, using a 2-D two component model (ambient medium and pulsar wind have different specific
heat ratios), 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 wound around the pulsar velocity direction. Moreover we estimate the opacity of the bow-shock
to penetration of ISM neutral hydrogen: this quantity affects observable properties of the nebula, like its size, shape, velocity
and surface brightness distribution. Finally we compare these numerical results with those from an analytical model. The development
of more realistic models is needed in order to tune the criteria for searches of new such objects, as well as to interpret
data on the known objects.
Key words: shock waves -- stars: pulsars: general -- stars: winds, outflows -- hydrodynamics -- methods: numerical
SIMBAD Objects
© ESO 2002
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