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Radio Physics and Radio Astronomy

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ISSN Druckformat: 2152-274X

ISSN Online: 2152-2758

SPECTRAL ENERGY DISTRIBUTION SIMULATIONS FOR SUBSTARS WITH GAPLESS DISKS

Volumen 2, Ausgabe 2, 2011, pp. 125-132
DOI: 10.1615/RadioPhysicsRadioAstronomy.v2.i2.50
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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.

REFERENZIERT VON
  1. Zakhozhay Olga, Dependence of Circumsubstellar Disk SEDs on System Inclination, Proceedings of the International Astronomical Union, 7, S282, 2011. Crossref

  2. Zakhozhay O., del Burgo C., Zakhozhay V., Geometry of highly inclined protoplanetary disks, Advances in Astronomy and Space Physics, 5, 1, 2015. Crossref

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