Asymmetric shapes of radio recombination lines from ionized stellar winds
Recombination line profile shapes are derived for ionized spherical stellar winds at radio wavelengths. It is assumed that the wind is optically thick owing to free-free opacity. Emission lines of arbitrary optical depth are obtained assuming that the free-free photosphere forms in the outer, consta...
Збережено в:
| Опубліковано в:: | Revista Mexicana de Astronomía y Astrofísica |
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| Автор: | |
| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
Universidad Nacional Autónoma de México
2019
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| Предмети: | |
| Онлайн доступ: | https://www.redalyc.org/articulo.oa?id=57171616005 https://www.redalyc.org/journal/571/57171616005/ https://www.redalyc.org/journal/571/57171616005/html/ https://www.redalyc.org/journal/571/57171616005/57171616005.epub https://www.redalyc.org/journal/571/57171616005/movil |
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