Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/969
Title: Stark broadening of O v 1371 Å line in stellar atmospheres
Authors: Dimitrijević, Milan S.
Kovačević, Anđelka 
Simić, Zoran
Dačič, Miodrag
Affiliations: Astronomy 
Keywords: Atomic processes;Line profiles;Stars;White dwarf
Issue Date: 22-Oct-2008
Related Publication(s): Exploring the Solar System and the Universe 2008
Journal: AIP Conference Proceedings
Abstract: 
The Stark broadening parameters of O V 1371 Å spectral line, observed in stellar atmospheres of hot stars, determined within the semiclassical perturbation method, are used for the analysis of the importance of this broadening mechanism in white dwarf atmospheres. We found that Stark broadening mechanism is very important in such plasma conditions and should be taken into account. © 2008 American Institute of Physics.
URI: https://research.matf.bg.ac.rs/handle/123456789/969
ISBN: 9780735405714
ISSN: 0094243X
DOI: 10.1063/1.2993686
Appears in Collections:Research outputs

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