Short-period line profile variations in the Be star μ Centauri

Monthly Notices of the Royal Astronomical Society

Volumn 324, Issue 4, 2001, Pages 1041-1053

  Balona, L A ^a   James, D J ^b   Lawson, W A ^c   Shobbrook, R R ^d  

^a SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

^c UNIVERSITY OF NEW SOUTH WALES   (Australia)

^d AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

Author keywords

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

Indexed keywords

PHOTOMETRY;

ABSORPTION FEATURES; BE STARS; CIRCUMSTELLAR; LINE: PROFILES; RESIDUAL ABSORPTION; SPECTRA'S; STAR: INDIVIDUAL: Μ CEN; STARS: EMISSION-LINE BE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:EARLY TYPE;

STARS;

EID: 0041461960     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04383.x     Document Type: Article

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