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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 12/1995, Volume 277, Issue 4, pp. 1547 - 1554
We review the correlation between the projected rotational velocity and the periods of the periodic Be stars (lambda Eri variables). By estimating the radius... 
stars, rotation | stars, variables, other | stars, oscillations | FREQUENCY NONRADIAL PULSATIONS | OBJECTS | SOUTHERN | stars, emission-line, Be | VARIABILITY | RAPIDLY ROTATING STARS | ASTRONOMY & ASTROPHYSICS | LINE-PROFILE VARIATIONS | INTENSIVE PHOTOMETRY | VARIABLES | NGC-3766
Journal Article
Astronomical Journal, ISSN 0004-6256, 1997, Volume 113, Issue 4, pp. 1359 - 1370
NGC 3766 is a young open cluster, located in the Carina complex, which contains an unusually large number of Be stars. This fact makes it specially interesting... 
LUMINOSITY FUNCTIONS | STAR-FORMATION PROCESS | EVOLUTION | MODELS | ASTRONOMY & ASTROPHYSICS | MASS | SOUTHERN CLUSTERS | NGC-3766 | UVBY-BETA-PHOTOMETRY | PROBES | RANGE | K BU ASTRONOMY & ASTROPHYSICS
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 08/1992, Volume 261, Issue 2, pp. 477 - 481
Using all available uvby observations we find that HR 5375, sigma-Lupi, and HR 6174 are small-amplitude, singly-periodic variables, having periods equal to... 
STARS, VARIABLE | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | STARS, EARLY-TYPE | PHOTOMETRIC VARIABILITY | STARS | NGC-3766 | STARS, INDIVIDUAL | SOUTHERN
Journal Article
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