Properties and nature of Be stars

Astronomy and Astrophysics

Volumn 506, Issue 3, 2009, Pages 1319-1333

  Ruzdjak D ^a   Bozic H ^a   Harmanec, P ^b   Firt R ^c   Chadima, P ^b   Bjorkman, K ^d   Gies, D R ^e   Kaye, A B ^f   Koubsky P ^g   McDavid, D ^h   Richardson, N ^e   Sudar, D ^a   Slechta M ^g   Wolf, M ^b   Yang, S ⁱ  

^a UNIVERSITY OF ZAGREB   (Croatia)

^b CHARLES UNIVERSITY   (Czech Republic)

^c UNIVERSITY OF BAYREUTH   (Germany)

^d UNIVERSITY OF TOLEDO   (United States)

^e GEORGIA STATE UNIVERSITY   (United States)

^f GEORGE MASON UNIVERSITY   (United States)

^g ASTRONOMICAL INSTITUTE   (Czech Republic)

^h UNIVERSITY OF VIRGINIA   (United States)

ⁱ UNIVERSITY OF VICTORIA   (Canada)

Author keywords

Binaries: spectroscopic; Stars: early type; Stars: emission line, Be; Stars: individual: Tauri

Indexed keywords

BE STARS; BINARIES: SPECTROSCOPIC; FOURIER TECHNIQUES; RADIAL VELOCITY; SPECTRAL REDUCTIONS; STARS: EARLY-TYPE; STARS: EMISSION-LINE, BE; STARS: INDIVIDUAL: TAURI; TIME VARIATIONS; TIME-SCALES;

PHOTOMETRY;

STARS;

EID: 70350780561     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200810526     Document Type: Article

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