Model atmospheres of chemically peculiar stars Self-consistent empirical stratified model of HD 24712

Astronomy and Astrophysics

Volumn 499, Issue 3, 2009, Pages 879-890

  Shulyak, D ^a   Ryabchikova, T ^a,b   Mashonkina, L ^b   Kochukhov, O ^c  

^a UNIVERSITY OF VIENNA   (Austria)

^b INSTITUTE OF ASTRONOMY   (Russian Federation)

^c UPPSALA UNIVERSITY   (Sweden)

Author keywords

Stars: Atmospheres; Stars: Chemically peculiar; Stars: Individual: Hd 24712

Indexed keywords

ATMOSPHERIC MODEL; CHEMICALLY PECULIAR-STARS; HIGH-RESOLUTION SPECTRA; INHOMOGENEITIES; INVERSE TEMPERATURES; ITERATIVE PROCEDURES; MAXIMUM TEMPERATURE; MINIMIZATION TOOLS; MODEL ATMOSPHERE; PHYSICAL MECHANISM; SELF-CONSISTENT MODEL; SPECTRAL LINE; STARS: ATMOSPHERES; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: HD 24712; STELLAR ATMOSPHERES; STELLAR MODEL ATMOSPHERES; STRATIFIED MODEL;

ATMOSPHERIC TEMPERATURE; CHEMICAL ANALYSIS; CHEMICAL ELEMENTS; CHEMICALS; NEODYMIUM; STARS; UPPER ATMOSPHERE;

ATMOSPHERIC SPECTRA;

EID: 66949112504     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911623     Document Type: Article

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