Pregled bibliografske jedinice broj: 1209926
Impact of Stark broadening on Co II spectral line modelling in hot stars
Impact of Stark broadening on Co II spectral line modelling in hot stars // European physical journal D : atomic, molecular and optical physics, 75 (2021), 4; 141, 5 doi:10.1140/epjd/s10053-021-00149-w (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 1209926 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Impact of Stark broadening on Co II spectral line
modelling in hot stars
Autori
Almodlej, Abeer ; Majlinger, Zlatko ; Ben Nessib, Nabil, Dimitrijević, S. Milan ; Srećković, A. Vladimi
Izvornik
European physical journal D : atomic, molecular and optical physics (1434-6060) 75
(2021), 4;
141, 5
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
Spectral line broadening, Stark width, hot stars atmosphere
(Spectral line broadening, Stark width, hot stars spectra, abundance determination)
Sažetak
The neglecting of Stark broadening in analysis and synthesis of hot stars spectra in some cases could cause errors in abundance determination. We analysed Co II lines in the spectrum of χ Lupi and found two well-isolated and strong lines (λ λ 2022.354, 2027.040 Å) suitable for the investigation of influence of Stark broadening. Since the results for both lines are qualitatively the same, we will discuss only for one of them. Comparisons of synthetic lines with and without taking of Stark broadening into consideration, in the case of the χ Lupi star and for the Co II lines, show that even when Stark width is negligible in comparison with Doppler width, Stark broadening may influence line wings.
Izvorni jezik
Engleski
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus