We report photoelectric UBV observations of four supergiants with larg
e infrared excesses: IRAS 18095+2704 and 19386+0155, and SAO 124414 an
d 34504. These are possible precursors of planetary nebula. All of the
m revealed brightness variations of 0.2m to 0.5m during the period fro
m 1990 to 1992.