On the influence of Stark broadening on Cri lines in stellar atmospheres

Astronomy and Astrophysics

Volumn 435, Issue 3, 2005, Pages 1191-1198

  Dimitrijevic M S ^a,b   Ryabchikova, T ^c,d   Popovic L C ^a,b,e   Shulyak, D ^f   Khan, S ^f  

^a ASTRONOMICAL OBSERVATORY   (Serbia)

^b Isaac Newton Institute of Chile   (Yugoslavia)

^c INSTITUTE OF ASTRONOMY   (Russian Federation)

^d UNIVERSITY OF VIENNA   (Austria)

^e ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^f TAURIDA NATIONAL V I VERNADSKY UNIVERSITY   (Ukraine)

Author keywords

Atomic processes; Line: profiles; Stars: chemically peculiar; Stars: individual: CrB

Indexed keywords

CALCULATIONS; DATA ACQUISITION; ELECTRONS; OPTIMIZATION; PERTURBATION TECHNIQUES; SPECTRUM ANALYSIS; THERMAL EFFECTS;

ATOMIC PROCESSES-LINE; CHEMICALLY PECULIAR-STARS; CRB; INDIVIDUAL; PROFILES-STARS;

EXTRATERRESTRIAL ATMOSPHERES;

EID: 19644395123     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042318     Document Type: Article

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