Short period line profile and light variations in the Be star ω Orionis

Monthly Notices of the Royal Astronomical Society

Volumn 327, Issue 4, 2001, Pages 1288-1296

  Balona, L A ^a   Aerts, C ^b   Bozic H ^c   Guinan, E F ^d   Handler, G ^a   James, D J ^e,f   Kaye, A B ^h   Shobbrook, R R ^g  

^a SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^b KU LEUVEN   (Belgium)

^c UNIVERSITY OF ZAGREB   (Croatia)

^d VILLANOVA UNIVERSITY   (United States)

^e UNIVERSITY OF ST ANDREWS   (United Kingdom)

^f UNIVERSITÉ DE GENÈVE   (Switzerland)

^g AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^h NONE

Author keywords

Line: profiles; Stars: early type; Stars: emission line, Be; Stars: individual: Ori

Indexed keywords

STARS;

ABSORPTION FEATURES; BE STARS; CIRCUMSTELLAR MATERIALS; LINE: PROFILES; PHOTOMETRICS; SHORT PERIODS; STAR: INDIVIDUAL: Ω ORI; STARS: EMISSION-LINE BE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:EARLY TYPE;

PHOTOMETRY;

EID: 0009752847     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04831.x     Document Type: Article

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