Atomic Line Widths by Thermal Energy Fluctuations in Stellar Atmospheres

Cardona O.

Vol. 40 No. 1 (2011), Contributions

Vol. 40 No. 1 (2011)

Contributions

Atomic Line Widths by Thermal Energy Fluctuations in Stellar Atmospheres

Cardona O.⁺⁻

Cardona O.

Instituto Nacional de Astrofísica, Óptica y Electrónica, Luis E. Erro 1, Tonantzintla, Puebla, 72840, Mexico

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Keywords

atomic processes
line: profiles
stars: atmospheres

How to Cite

Atomic Line Widths by Thermal Energy Fluctuations in Stellar Atmospheres. (2011). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 40(1), 227-228. https://astronomia.unam.mx/journals/rmxac/article/view/2011rmxac..40..227c

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Abstract

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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Atomic Line Widths by Thermal Energy Fluctuations in Stellar Atmospheres

Keywords

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