  Recent studies using 21 cm HI line and $^{13}$CO line observations in the
inner part of the Galaxy have resulted in new distances for 30 Galactic
supernova remnants (SNRs). 15 of those remnants have observed X-ray spectra,
for which shocked-gas temperatures and emission measures are measured. Here we
apply spherically symmetric SNR evolution models to these 15 remnants to obtain
estimates for ages, explosion energies, circum-stellar medium densities and
profiles (uniform or wind-type).From the distribution of ages we obtain a
supernova birth rate and estimate incompleteness. The energies and densities
can be well fit with log-normal distributions. The distribution of explosion
energies is very similar to that of SNRs in the Large Magellanic Cloud (LMC),
suggesting SN explosions in the LMC and in the Galaxy are very similar. The
density distribution has higher mean density for Galactic SNRs than for LMC
SNRs, by a factor $\sim$2.5.
