Multicomponent radiatively driven stellar winds IV. On the helium decoupling in the wind of σ Orionis E

Astronomy and Astrophysics

Volumn 460, Issue 1, 2006, Pages 145-153

  Krticka J ^a   Kubat J ^b   Groote, D ^c  

^a MASARYK UNIVERSITY   (Czech Republic)

^b ASTRONOMICAL INSTITUTE   (Czech Republic)

^c UNIVERSITY OF HAMBURG   (Germany)

Author keywords

Hydrodynamics; Stars: chemically peculiar; Stars: early type; Stars: mass loss; Stars: winds, outflows

Indexed keywords

HELIUM; HYDRODYNAMICS; MAGNETIC FIELDS; MATHEMATICAL MODELS; SOLAR SYSTEM; SPACE HEATING;

STARS: CHEMICALLY PECULIAR; STARS: EARLY-TYPE; STARS: MASS-LOSS; STARS: WINDS, OUTFLOWS;

GALAXIES;

EID: 33845327178     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065128     Document Type: Article

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