The Optical Gravitational Lensing Experiment (OGLE) is a long term
project with the main goal of searching for dark matter in our Galaxy by
identifying microlensing events toward the galactic bulge (Udalski et
al. 1992, 1994). At times the Bulge is unobservable we conduct
other long-term photometric programs.
A complete list of side-projects attempted by the OGLE team
can be found in Paczynski et al. (1995).
In particular, during last three observing seasons we monitored globular
clusters NGC 104 (=47 Tuc) and NGC 5139 (
) in a
search for variable stars of various types. Of primary interest was
detection of detached eclipsing binaries. In Paper I (Kaluzny et al.
1996) we presented results for three fields in 
.
Here we report on variables discovered in another three fields of that
cluster.