  In this work is examined a new modeling way of describing the continuous
absorption of electromagnetic (EM) radiation in a dense partially ionized
hydrogen plasmas with electron densities about $5\cdot10^{18}$ cm$^{-3}$ -
$1.5\cdot10^{19}$cm$^{-3}$ and temperatures about $1.6 \cdot10^{4}$ K - $2.5
\cdot 10^{4}$ K in the wavelength region $300 \textrm{nm} < \lambda < 500
\textrm{nm}$. The obtained results can be applied to the plasmas of the
partially ionized layers of different stellar atmospheres.
