Atomic Line Widths by Thermal Energy Fluctuations in Stellar Atmospheres

Details Atomic Line Widths by Thermal Energy Fluctuations in Stellar Atmospheres Atomic Line Widths by Thermal Energy Fluctuations in Stellar Atmospheres

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..227c&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Atomic Processes, Line: Profiles, Stars: Atmospheres

Scientific paper

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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