Stark broadening of Zr IV spectral lines in the atmospheres of chemically peculiar stars (CROSBI ID 261356)
Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Majlinger, Zlatko ; Simić, Zoran ; Dimitrijević, Milan S.
engleski
Stark broadening of Zr IV spectral lines in the atmospheres of chemically peculiar stars
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.
atomic data, atomic processes, line: formation
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
Podaci o izdanju
470 (2)
2017.
1911-1918
objavljeno
0035-8711
1365-2966
10.1093/mnras/stx1321