Properties and nature of Be stars: 29. Orbital and long-term spectral variations of γ Cassiopeiae

Astronomy and Astrophysics

Volumn 537, Issue , 2012, Pages

  Nemravova J ^a   Harmanec, P ^a   Koubsky P ^b   Miroshnichenko, A ^c   Yang, S ^d   Slechta M ^b   Buil, C ^e   Korcakova D ^a   Votruba, V ^b  

^a CHARLES UNIVERSITY   (Czech Republic)

^b ASTRONOMICAL INSTITUTE   (Czech Republic)

^c UNIVERSITY OF NORTH CAROLINA AT GREENSBORO   (United States)

^d UNIVERSITY OF VICTORIA   (Canada)

^e Association des Utilisateurs de Détecteurs Électroniques AUDE   (France)

Author keywords

binaries: spectroscopic; stars: early type; stars: emission line, Be

Indexed keywords

ANTICORRELATION; BE STARS; BINARIES: SPECTROSCOPIC; CIRCUMSTELLAR ENVELOPES; EMISSION LINES; HIGH-RESOLUTION SPECTRA; LOW-MASS; ORBITAL ELEMENT; PEAK INTENSITY; SPECTRAL OBSERVATIONS; SPECTRAL VARIATION; STARS: EARLY-TYPE; STARS: EMISSION-LINE , BE; TIME DISTRIBUTION; TIME INTERVAL;

SPECTROSCOPIC ANALYSIS;

STARS;

EID: 84862927523     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117922     Document Type: Article

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