a period of 11.05 hours. Spectroscopic data were presented by Carrier and Burki which suggest that during the brightness outbursts, "blobs" of ejected matter can be detected moving through a Keplerian disk surrounding the star. References 032385 049131 Canis Majoris, HP Emission-line stars Be stars Lambda Eridani variables Gamma Cassiopeiae variable stars B-type main-sequence stars 2501