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ISSN Druckformat: 2152-274X
ISSN Online: 2152-2758
SPECTRAL ENERGY DISTRIBUTION SIMULATIONS FOR SUBSTARS WITH GAPLESS DISKS
ABSTRAKT
An algorithm is presented to calculate the spectral energy distributions of substars with gapless disks depending on their geometry, age and angle of observation. 336 spectral energy distributions have been calculated in the systems spaced within 10 pc and consisting of a substar with mass (0.01−0.08)Mʘ , aged 1−30 Myr, and a flat or flared gapless disk observed at angles of 0° to 80° . The emission fluxes from such systems are > 0.001 Jy at wavelengths from 1.7 μm to 1 cm, while at wavelengths > 40 μm the fluxes from disks, irrespective of angle of observation, are determinant in the total emission of systems.
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