On the role of duplicity in the Be phenomenon. I. General considerations and the first attempt at a 3-D gas-dynamical modelling of gas outflow from hot and rapidly rotating OB stars in binaries

Astronomy and Astrophysics

Volumn 396, Issue 3, 2002, Pages 937-948

  Harmanec, P ^a,b   Bisikalo, D V ^c   Boyarchuk, A A ^c   Kuznetsov, O A ^d  

^a CHARLES UNIVERSITY   (Czech Republic)

^b ASTRONOMICAL INSTITUTE   (Czech Republic)

^c INSTITUTE OF ASTRONOMY   (Russian Federation)

^d KELDYSH INSTITUTE OF APPLIED MATHEMATICS   (Russian Federation)

Author keywords

Stars: binaries: close; Stars: binaries: spectroscopic; Stars: emission line, Be; Stars: fundamental parameters

Indexed keywords

COMPUTER SIMULATION; GAS DYNAMICS; GAS METERS; INTERFEROMETRY; NUMERICAL ANALYSIS; VELOCITY;

BINARY COMPONENTS;

ASTROPHYSICS;

EID: 0036907488     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021534     Document Type: Article

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