Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...92..533b&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 92, no. 3, Feb. 1992, p. 533-563.
Astronomy and Astrophysics
Astrophysics
45
Astronomical Photometry, B Stars, Southern Sky, Variable Stars, Late Stars, Periodic Variations, Stellar Oscillations, Stellar Rotation, Summer
Scientific paper
Results are presented of photometric campaign on some bright southern Be stars to search for periodic light variations. In order to obtain good phase coverage, many observations were conducted from two sites with different longitudes: ESO and SAAO. A large fraction of early-Be stars are found to be variable with periods close to or equal to their rotational periods. Particular attention is devoted to the late-Be stars. Unlike the hotter members of this class, the late-Be stars do not seem to have detectable periodic light variations except for one or two stars of very small amplitude.
Balona Luis A.
Cuypers Jan
Marang Freddy
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