Stark broadening of hydrogen Lyman and Balmer in the conditions of stellar envelopes

Details Stark broadening of hydrogen Lyman and Balmer in the conditions of stellar envelopes Stark broadening of hydrogen Lyman and Balmer in the conditions of stellar envelopes

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26as..104..509s&link_type=abstract

Astronomy and Astrophysics Suppl. 104, 509-527 (1994)

Astronomy and Astrophysics

Astrophysics

44

Atomic Data, Atomic Processes, Lines Profiles

Scientific paper

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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