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...
-д хадгалсан:
| -д хэвлэсэн: | Revista Mexicana de Astronomía y Astrofísica |
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| Үндсэн зохиолч: | |
| Формат: | Artigo |
| Хэл сонгох: | Inglês |
| Хэвлэсэн: |
Universidad Nacional Autónoma de México
2000
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| Нөхцлүүд: | |
| Онлайн хандалт: | https://www.redalyc.org/articulo.oa?id=57100973 |
| Шошгууд: |
Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!
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