Volume 425, Number 3, October III 2004
|Page(s)||1147 - 1152|
|Section||Atomic, molecular, and nuclear data|
|Published online||28 September 2004|
Stark broadening of Ga I spectral lines*
Astronomical Observatory, Volgina 7, 11160 Belgrade, Serbia and Montenegro e-mail: firstname.lastname@example.org
2 Institute Isaac Newton of Chile, Yugoslavia Branch
Accepted: 10 May 2004
Stark broadening of the 18 Ga I transitions has been analyzed within the framework of the semiclassical perturbation method. Results obtained have been compared with available experimental and theoretical data and used for the consideration of the influence of the Stark broadening effect in stellar atmospheres
Key words: line: profiles / atomic data / atomic processes / line: formation / stars: atmospheres
© ESO, 2004
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