Models of the magnetic field evolution in supernova remnants

Details Models of the magnetic field evolution in supernova remnants Models of the magnetic field evolution in supernova remnants

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006pobeo..80...95v&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, Vol. 80, p. 95-97

Astronomy and Astrophysics

Astronomy

1

Supernova Remnants

Scientific paper

In this paper we present a brief discussion of the magnetic field (H) evolution in supernova remnant (SNRs). Evolution models generally assume H ∝ D-δ. Knowing δ would be particularly important in the study of the radio surface brightness to diameter (Σ -D) relation for SNRs, since it would allow us to compare different theoretical models for the radio evolution.

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