Nonequilibrium ionization models for analysis of x-ray spectra of supernova remnants
Among the brightest sources of X-ray emission are supernova remnants(SNRs), which will be extensively observed by new X-ray satellites (Chandra, XMM,and Astro-E). Thermal X-ray emission from SNRs cannot be analyzed with stan-dard X-ray plasma codes, because plasmas in these objects are not in ioniza...
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Hovedforfatter: | |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2000
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| Online adgang: | https://www.redalyc.org/articulo.oa?id=57100973 |
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