On the Stark broadening of Te I spectral lines for CP star plasma analysis

Contributions of the Astronomical Observatory Skalnate Pleso

Volumn 38, Issue 2, 2008, Pages 403-404

  Dimitrijevic M S ^a   Simic Z ^a   Kovacevic A ^b   Dacic M ^a   Sahal Brechot S ^c  

^a Astronomical Observatory   (Serbia)

^b Faculty of Mathematics   (Serbia)

^c OBSERVATOIRE DE PARIS   (France)

Author keywords

Atomic data; Atomic processes; Line: formation; Line: profiles; Stars: atmospheres; Stars: chemically peculiar

Indexed keywords

EID: 45749114184     PISSN: 13351842     EISSN: 13360337     Source Type: Journal    
DOI: None     Document Type: Conference Paper

References (6)

1. Chayer, P., Vennes, S., Dupuis, J., Kruk, J.W.: 2005, Astrophys. J. 630, L169
2. Dimitrijević, M.S.: 1996, Zh. Priklad. Spektrosk. 63, 810
3. Kurucz, R.L.: 1979, Astrophys. J., Suppl. Ser. 40, 1
4. Sahal-Bréchot, S.: 1969 a, Astron. Astrophys. 1, 9
5. Sahal-Bréchot, S.: 1969 b, Astron. Astrophys. 2, 322
6. Yuschenko, AN., Gopka, V.F.: 1996, Astron. Astrophys. Transaction 10, 307