The intrinsic high metallicity of cSNRs

Abstract

Here we present semi-analytical solutions of the hydrodynamics of compact supernova remnants (cSNRs) and their chemical evolution. Two models of $15M_{\odot }$ and $25M_{\odot }$ supernova explosions evolving in a high density medium ($n_0\sim 10^{7}c{m}^{-3}$) are throughly discussed.

4 pages, 3 figures, Accepted for publication in Revista Mexicana de Astronomia & Astrofisica