Photometric and spectroscopic studies of star-forming regions within
  Wolf-Rayet galaxies
  We present a study of the properties of star-forming regions within a sample
of 7 Wolf-Rayet (WR) galaxies. We analyze their morphologies, colours,
star-formation rate (SFR), metallicities, and stellar populations combining
broad-band and narrow-band photometry with low-resolution optical spectroscopy.
The $UBVRI$ observations were made through the 2m HCT (Himalayan Chandra
Telescope) and 1m ARIES telescope. The spectroscopic data were obtained using
the Hanle Faint Object Spectrograph Camera (HFOSC) mounted on the 2m HCT. The
observed galaxies are NGC 1140, IRAS 07164+5301, NGC 3738, UM 311, NGC 6764,
NGC 4861 and NGC 3003. The optical spectra have been used to search for the
faint WR features, to confirm that the ionization of the gas is consequence of
the massive stars, and to quantify the oxygen abundance of each galaxy using
several and independent empirical calibrations. We detected the broad features
originated by WR stars in NGC 1140 and NGC 4861 and used them to derive their
population of massive stars. Using our H$\alpha$ images we have identified tens
of regions within these galaxies, for which we derived the SFR. For all regions
we found that the most recent star-formation event is 3 - 6 Myr old. We used
the optical broad-band colours in combination with Starburst99 models to
estimate the internal reddening and the age of the dominant underlying stellar
population within all these regions. Knots in NGC 3738, NGC 6764 and NGC 3003
generally show the presence of an important old (400 - 1000 Myr) stellar
population. However, the optical colours are not able to detect stars older
than 20 - 50 Myr in the knots of the other four galaxies. This fact suggests
both the intensity of the starbursts and that the star-formation activity has
been ongoing for at least some few tens of million years in these objects.
