  It has recently been reported that some of the flux density values for an
evolved supernova remnant (SNR) HB 3 (G132.7 + 1.3) are not accurate. In this
work we revised an analysis of the possible thermal emission at radio
frequencies from the SNR HB 3 using the recently published, corrected, flux
density values. A model including a sum of non-thermal (purely synchrotron) and
thermal (bremsstrahlung) component is applied for fitting integrated radio
spectrum of the SNR. The contribution of thermal component in total volume
emissivity at $1 \mathrm{GHz}$ was estimated to be $\approx37 %$. The ambient
density was also estimated to be $n\approx 9 \mathrm{cm}^{-3}$ for the
$\mathrm{T}=10^{4} \mathrm{K}$. Again, we obtained the relatively significant
presence of thermal emission at radio frequencies from the SNR so we could
support interaction between SNR HB 3 and adjacent molecular cloud associated
with the H {\sc ii} region W3. Our model estimates for thermal component
contribution to total volume emissivity at $1 \mathrm{GHz}$ and ambient density
are similar to those obtained earlier ($\approx40 %$, $\approx10
\mathrm{cm^{-3}}$). It is clear that the corrected flux density values do not
change the basic conclusions.
