Properties and nature of Be stars: 25. A new orbital solution and the nature of a peculiar emission-line binary v Sagittarii

Astronomy and Astrophysics

Volumn 459, Issue 3, 2006, Pages 849-857

  Koubsky P ^a   Harmanec, P ^a,b   Yang, S ^c   Netolicky M ^a,d   Skoda P ^a   Slechta M ^a   Korcakova D ^a  

^a ASTRONOMICAL INSTITUTE   (Czech Republic)

^b CHARLES UNIVERSITY   (Czech Republic)

^c UNIVERSITY OF VICTORIA   (Canada)

^d MASARYK UNIVERSITY   (Czech Republic)

Author keywords

Stars: binaries: close; Stars: emission line, Be; Stars: individual: v sagittarii

Indexed keywords

ABSORPTION; INTERFEROMETRY; OPTICAL RESOLVING POWER; ORBITS; PHOTOMETRY; PROBABILITY;

MASS EXCHANGE; STARS: BINARIES: CLOSE; STARS: EMISSION LINE; STARS: INDIVIDUAL: V SAGITTARII;

GALAXIES;

EID: 37849186997     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065274     Document Type: Article

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