| Issue |
A&A
Volume 425, Number 3, October III 2004
|
|
|---|---|---|
| Page(s) | 1147 - 1152 | |
| Section | Atomic, molecular, and nuclear data | |
| DOI | https://doi.org/10.1051/0004-6361:20047066 | |
| Published online | 28 September 2004 | |
Stark broadening of Ga I spectral lines*
1
Astronomical Observatory, Volgina 7, 11160 Belgrade, Serbia and Montenegro e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
2
Institute Isaac Newton of Chile, Yugoslavia Branch
Received:
13
January
2004
Accepted:
10
May
2004
Abstract
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
Table [see full text] is also available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/425/1147
© ESO, 2004
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