The intrinsic high metallicity of cSNRs

Authors:
A. Rodriguez-Gonzalez,
G. Tenorio-Tagle,
S. Silich

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

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.

References and citations for this submission:

SLAC-SPIRES HEP (refers to ,
cited by, arXiv reformatted)