ATOMIC LINE WIDTHS BY THERMAL ENERGY FLUCTUATIONS IN STELLAR ATMOSPHERES
A method for finding the width of the atomic lines using the thermal energy fluctuations is presented in this work. Comparisons are made with published experimental and theoretical values.
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2011
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57121297116 |
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