Magnetic model for asymmetric supernova remnants

Details Magnetic model for asymmetric supernova remnants Magnetic model for asymmetric supernova remnants

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...355l..47m&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 355, June 1, 1990, p. L47-L50. Research supported by the Robert A

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Astronomical Models, Interstellar Matter, Supernova Remnants, Density Distribution, Interstellar Magnetic Fields, Magnetohydrodynamics

Scientific paper

Results are reported from two-dimensional MHD simulations for the asymmetric SNRs such as VRO 42.05.01. Two models are compared: one is the hot tunnel model, in which the hot elongated cavity (tunnel) between two warm interclouds is responsible for the observed asymmetric structure. The other is the magnetic model, in which material from the warm intercloud is compresed by the SN shock at the magnetic wall, creating an arc-shaped dense structure. The shapes of the density contours are quite similar. In contrast, the velocity vectors differ significantly between the two models.

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