Stark broadening of Zr iv spectral lines in the atmospheres of chemically peculiar stars
Autor: | Zlatko Majlinger, Milan S. Dimitrijević, Zoran Simić |
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Přispěvatelé: | Astronomical Observatory Belgrade (AOB), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS-PSL) |
Jazyk: | angličtina |
Rok vydání: | 2017 |
Předmět: |
Physics
[PHYS]Physics [physics] atomic data atomic processes line: formation Astronomy and Astrophysics Astrophysics 01 natural sciences Spectral line symbols.namesake Stars Stark effect Space and Planetary Science 0103 physical sciences symbols Physics::Atomic Physics 010306 general physics [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] 010303 astronomy & astrophysics ComputingMilieux_MISCELLANEOUS Atomic data |
Zdroj: | Monthly Notices of the Royal Astronomical Society Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 470 (2), pp.1911-1918. ⟨10.1093/mnras/stx1321⟩ Monthly Notices of the Royal Astronomical Society, 2017, 470 (2), pp.1911-1918. ⟨10.1093/mnras/stx1321⟩ |
ISSN: | 0035-8711 1365-2966 |
Popis: | Stark widths for 18 Zr IV spectral lines have been calculated by using the modified semi-empirical method. The obtained results have been used to investigate the influence of Stark broadening on the spectra of atmospheres of chemically peculiar stars of A spectral type and hydrogen-rich DA and helium-rich DB white dwarfs. Our results have been used also to test possibility to predict new data using some approximate methods developed on the basis on regularities and systematic trends. |
Databáze: | OpenAIRE |
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