Observations of the Leo A dwarf galaxy, obtained over the period from
1980 to 1991 are reported. Forty two separate CCD frames were searched
for variable stars. A total of 14 suspected variables were found, 9 h
ad sufficient coverage for period determination, and 5 had Cepheid lig
ht curves. Four of these stars fit well on a P-L relation and yield a
distance modulus, after correction for Galactic foreground extinction,
of m - M = 26.74. This corresponds to a distance of 2.2 Mpc, placing
Leo A near the Local Group zero-velocity surface.