New $ubvri$ photometry of 234 M33 star clusters
  This is the second paper of our series. In this paper, we present $UBVRI$
photometry for 234 star clusters in the field of M33. For most of these star
clusters, there is photometry in only two bands in previous studies. The
photometry of these star clusters is performed using archival images from the
Local Group Galaxies Survey, which covers 0.8 deg$^2$ along the major axis of
M33. Detailed comparisons show that, in general, our photometry is consistent
with previous measurements, especially, our photometry is in good agreement
with Zloczewski & Kaluzny. Combined with the star clusters' photometry in
previous studies, we present some results: none of the M33 youngest clusters
($\sim 10^7$ yr) have masses approaching $10^5$ $M_{\odot}$; comparisons with
models of simple stellar populations suggest a large range of ages of M33 star
clusters, and some as old as the Galactic globular clusters.
