Stark broadening of Zr iv spectral lines in the atmospheres of chemically peculiar stars

Autor: Zlatko Majlinger, Milan S. Dimitrijević, Zoran Simić
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:
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