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Radio Physics and Radio Astronomy

Publicou 4 edições por ano

ISSN Imprimir: 2152-274X

ISSN On-line: 2152-2758

SPECTRAL ENERGY DISTRIBUTION SIMULATIONS FOR SUBSTARS WITH DISKS HAVING INNER HOLES

Volume 2, Edição 3, 2011, pp. 211-220
DOI: 10.1615/RadioPhysicsRadioAstronomy.v2.i3.30
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RESUMO

An algorithm of spectral energy distribution simulations has been developed for substars and disks with inner holes as a dependence of their geometry, age and inclination angle. Calculated are 560 spectral energy distributions of systems located at 10 pc and consisting of substar with mass (0.01 − 0.08)M, age (1 − 30) Myr and flat or flaring disk with inner hole and inclined at angles 0° − 80°. Basic regularities of flux variation with ages and central object masses are analyzed. The data obtained are compared with those for fluxes from the systems without inner hole.

CITADO POR
  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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