C. Stehlé
Abstract
Tables of Stark broadened hydrogen lines of the Lyman and Balmer series are presented under the conditions of stellar envelopes. The formalism is based on the Model Microfield Method (MMM) for both the electronic and ionic contributions to the line shape
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Tables of Stark broadened hydrogen lines of the Lyman and Balmer series are presented under the conditions of stellar envelopes. The formalism is based on the Model Microfield Method (MMM) for both the electronic and ionic contributions to the line shape
Key concepts: Balmer series, Physics, Stark effect, Hydrogen spectral series, Hydrogen line, Stellar atmosphere, Astrophysics, Formalism (music)