Abstract:
The present paper is devoted to modeling of radiative heat
transfer in forming planetary systems. The solution of transfer
equation for dusty media of spherical polydispersive silicate
particles is considered.
An algorithm of computation of temperature distribution in
circumstellar disks is proposed. Coincidence of numerical results
and known analytical cases is shown. Spatial distribution of
optical characteristics of $\beta$-Pictoris debris disk are
obtained.
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