Stark broadening of O V 1371 A line in stellar atmospheres

Stark broadening of O V 1371 A line in stellar atmospheres

The Stark broadening parameters of O V 1371 A 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 mech...

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Hauptverfasser: Dimitrijevic, Milan S, Kovacevic, Andjelka, Simic, Zoran, Dacic, Miodrag
Format: Tagungsbericht
Sprache:eng
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Zusammenfassung:The Stark broadening parameters of O V 1371 A 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.
ISSN:0094-243X
DOI:10.1063/1.2993686