Optical photometric observations of the blazar OI 090.4 are presented
as part of an ongoing study of variations in blazars occurring on time
scales of minutes to hours, which has been termed microvariability. T
he observations presented here reveal the existence of such variabilit
y for this blazar and provide further evidence of the class-wide natur
e of this phenomenon. Time scales as short as these provide important
clues about the nature of blazars, and a discussion of the types of po
ssible mechanisms responsible for producing these variations is given.
(C) 1997 American Astronomical Society.