The Intrinsic High Metallicity of cSNRs
Here we present semi-analytical solutions of the hydrodynamics of compact supernova remnants (cSNRs) and their chemical evolution. Two models of 15 M๏ and 25 M๏ supernova explosions evolving in a high density medium (n0~107 cm-3) are throughly discussed. We demonstrate, that after a few...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2003
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57101827 |
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