Radio Observations of SNR Environments
Most supernova remnants (SNRs) in our Galaxy are expected to be close to their parent molecular clouds. Theinteraction between SNRs and interstellar clouds not only alter the morphology and evolution of a SNR but alsoheat, compress, disrupt or modify the chemistry of the cloud. The turbulence genera...
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| Publié dans: | Revista Mexicana de Astronomía y Astrofísica |
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| Auteur principal: | |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
Universidad Nacional Autónoma de México
2007
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| Sujets: | |
| Accès en ligne: | https://www.redalyc.org/articulo.oa?id=57130004 |
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