Photometric Monitoring of Bright Be Stars. III. 1988-89 and 1992-95

We report long-term photometric (BV) observations of 23 bright, active Be stars made in 1988 and 1989 and 1992 and 1995 with the 0.4m telescope at the University of Toronto. Cumulative light curves, including observations made earlier at the University of Toronto, and with the Automatic Photometric Telescope Service in Arizona, are presented for several of the stars. Many of the stars show cyclic variations of up to 0.2 in V and B on time scales of a few years, as well as variations on time scales of about a day. (SECTION: Stars)