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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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2003
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57101827 |
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