  We present an improved version of a light curve model, which is able to
estimate the physical properties of different types of core-collapse supernovae
having double-peaked light curves, in a quick and efficient way. The model is
based on a two-component configuration consisting of a dense, inner region and
an extended, low-mass envelope. Using this configuration, we estimate the
initial parameters of the progenitor via fitting the shape of the
quasi-bolometric light curves of 10 SNe, including Type IIP and IIb events,
with model light curves. In each case we compare the fitting results with
available hydrodynamic calculations, and also match the derived expansion
velocities with the observed ones. Furthermore, we also compare our
calculations with hydrodynamic models derived by the SNEC code, and examine the
uncertainties of the estimated physical parameters caused by the assumption of
constant opacity and the inaccurate knowledge of the moment of explosion.
