The intrinsic high metallicity of cSNRs

Details The intrinsic high metallicity of cSNRs The intrinsic high metallicity of cSNRs

2003-03-13

arxiv.org/abs/astro-ph/0303276v1

Astronomy and Astrophysics

Astrophysics

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

Scientific paper

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

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