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...
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 第一著者: | |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2007
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57130004 |
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