The evolution of compact supernova remnants in a strongly magnetized medium

Details The evolution of compact supernova remnants in a strongly magnetized medium The evolution of compact supernova remnants in a strongly magnetized medium

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.274.1157r&link_type=abstract

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

Astronomy and Astrophysics

Astronomy

3

Ism: Jets And Outflows, Ism: Magnetic Fields, Supernova Remnants, Galaxies: Active

Scientific paper

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.

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