Photoionization of galactic halo gas by old supernova remnants
We present new calculations on the contribution from cooling hot gas in oldsupernova remnants to the photoionization of warm ionized gas in the Galaxy. Weshow that the emission from the hot gas in cooling supernova remnants (SNRs)is soft ( E 20 eV) and, as a result, the eciency of conversion of su...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autore principale: | |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2000
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57100963 |
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