The radial distribution of radio emission from SN1993J: Magnetic field amplification due to the Rayleigh-Taylor instability

I. Marti-Vidal, C-I. Bjornsson, M. A. Perez-Torres +2

[SHORTENED VERSION] Observations of radio emission from young core-collapse supernovae (CCSNe) allow one to study the history of the pre-supernova stellar wind, trace the density s…