Continuous Spectra Calculation for Substars Possessing Disks with Inner Holes

Abstract

The algorithm of spectral energy distribution simulation for substars and disks with inner hole has been developed versus their geometry, age and inclination angle. Calculations are made for 560 spectral energy distributions of systems spaced 10 pc apart, consisting of substars with mass (0.01÷0.08)M and aged (1÷30) Мyr, and a flat or flaring disk with inner hole and inclined at angles 0°÷80°. Main regularities of flux changing are analyzed versus age and central object mass. The data obtained are compared with those for the systems without inner holes.