Stark Broadening of in III Lines in Astrophysical and Laboratory Plasma

Simic, Zoran J and Dimitrijevic, Milan S and Kovacevic, Andjelka B and Sahal-Brechot, S (2011) Stark Broadening of in III Lines in Astrophysical and Laboratory Plasma. Baltic Astronomy, 20 (4). pp. 613-617. ISSN 1392-0049 (FP7- 239108)

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Abstract

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.

Keywords

stars atmospheres; spectral lines; Stark broadening

Item Type:	Article
FP7 Grant Agreement Number:	239108
FrameWork Programmes:	SP4-Capacities
Scientific Areas:	Research Infrastructures
Contact Email Address:	zsimic@aob.bg.ac.rs
Last Modified:	08 Aug 2012 09:53
Access rights:	Open access
URI:	http://eprints.kobson.nb.rs/id/eprint/17

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