  A method for identification of stellar complexes in M33 is applied. Several
OB associations form a stellar complex with mean size of 0.3 - 1 kpc. We apply
a correlation technique to compare different stellar populations in M33. Our
results confirm the existence of a strong correlation between OB stars, HII
regions and WR stars, which trace the regions of massive star formation. There
is a good correlation between red supergiants (RSGs) and WR stars in the spiral
arms of M33. This can be expected since the progenitors of WR stars are massive
OB stars or RSGs with masses greater than 20 M_sun. The massive RSGs and WR
stars probably originate from nearby sites of star formation. We consider this
fact as a ground for identification of stellar complexes in M33. The presented
method for identification of stellar complexes can be applied to other nearby
galaxies.
