Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2012-01-10
Baltic Astronomy, vol. 20, 613-617, 2011
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientific paper
Besides the need of Stark broadening parameters for a number of problems in physics, and plasma technology, in hot star atmospheres the conditions exist where Stark widths are comparable and even larger than the thermal Doppler widths. Using the semiclassical perturbation method we investigated here the influence of collisions with charged particles for In III spectral lines. We determined a number of Stark broadening parameters important for the investigation of plasmas in the atmospheres of A-type stars and white dwarfs. Also, we have compared the obtained results with existing experimental data. The results will be included in the STARK-B database, the Virtual Atomic and Molecular Data Center and the Serbian Virtual Observatory.
Dimitrijevic Milan S.
Kovačević Andjelka B.
Sahal-Bréchot Sylvie
Simic Zoran
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