The evolution of compact supernova remnants in a strongly magnetized medium

Bibcode
1995MNRAS.274.1157R
Rozyczka, Michal; Tenorio-Tagle, Guillermo
Referencia bibliográfica

Monthly Notices of the Royal Astronomical Society, Volume 274, Issue 4, pp. 1157-1164.

Fecha de publicación:
6
1995
Revista
Monthly Notices of the Royal Astronomical Society
Número de autores
2
Número de autores del IAC
1
Número de citas
7
Número de citas referidas
7
Descripción
Two-dimensional simulations of the evolution of supernova remnants in a uniform, high-density medium are presented. The medium is magnetized, and its magnetic pressure is much larger than the thermal pressure. The evolution of the remnants is followed past full thermalization of the ejecta. A mechanism of self-collimation of the flow is identified, resulting in formation of jets that propagate along the magnetic field lines.
Tipo
Con árbitro
Campos magnéticos
Restos de supernova
Galaxias

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