Properties and nature of Be stars: 28. Implications of systematic observations for the nature of the multiple system with the Be star o Cassiopæ and its circumstellar environment

Astronomy and Astrophysics

Volumn 517, Issue 3, 2010, Pages

  Koubsky P ^a   Hummel, C A ^b   Harmanec, P ^c   Tycner, C ^d   Van Leeuwen, F ^e   Yang, S ^f   Slechta M ^a   Bozic H ^g   Zavala, R T ^h   Ruzdjak D ^g   Sudar, D ^g  

^a ASTRONOMICAL INSTITUTE   (Czech Republic)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c CHARLES UNIVERSITY   (Czech Republic)

^d CENTRAL MICHIGAN UNIVERSITY   (United States)

^e UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^f UNIVERSITY OF VICTORIA   (Canada)

^g UNIVERSITY OF ZAGREB   (Croatia)

^h US NAVAL OBSERVATORY   (United States)

Author keywords

Binaries: close; Binaries: spectroscopic; Stars: emission line, Be; Stars: fundamental parameters; Stars: individual: o Cas

Indexed keywords

BUILDINGS; CHEMICAL DETECTION; OBSERVATORIES; OPTICAL PROPERTIES; ORBITAL LABORATORIES;

ASTROPHYSICAL OBSERVATORY; BE STARS; BINARIES: CLOSE; BINARIES: SPECTROSCOPIC; BINARY COMPONENTS; BINARY SYSTEMS; CIRCUMSTELLAR; MASS FUNCTIONS; MULTIPLE SYSTEMS; NAVY PROTOTYPE OPTICAL INTERFEROMETERS; OPTICAL SPECTRA; ORBITAL PARAMETERS; RADIAL VELOCITY; SPATIALLY RESOLVED; STARS: INDIVIDUAL;

STARS;

EID: 77955078177     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014477     Document Type: Article

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