Stark broadening of H lines (Stehle 1995)

Details Stark broadening of H lines (Stehle 1995) Stark broadening of H lines (Stehle 1995)

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ycat.6082....0s&link_type=abstract

VizieR On-line Data Catalog: VI/82. Originally published in: 1994A&AS..104..509S

Physics

Atomic Physics

81

Atomic Physics

Scientific paper

Tables of Stark broadened hydrogen lines of the Lyman, Balmer and Paschen series are presented under the conditions of stellar envelopes. The formalism is based on the Model Microfield Method (MMM) (Brissaud and Frisch, Frisch and Brissaud 1971) for both the electronic and ionic contributions to the line shape. The range of temperatures is 10000 to 80000 K, and electronic densities between 3.2E+14 and 3.2E+16 cm-3. Lyman and Balmer results were published in A&AS 104, 509, whereas Paschen results were presented at the 1995 July Workshop in Vienna. (3 data files).

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