Modeling of SEDs for substars with disks that have different geometrical and physical parameters

Details Modeling of SEDs for substars with disks that have different geometrical and physical parameters Modeling of SEDs for substars with disks that have different geometrical and physical parameters

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..276..467z&link_type=abstract

The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution, Proceedings of the International Astronomi

Astronomy and Astrophysics

Astrophysics

Circumstellar Matter, Stars: Low-Mass, Brown Dwarfs, Planetary Systems: Protoplanetary Disks

Scientific paper

The algorithm of spectral energy distribution (SED) calculations for
protoplanetary disks and central objects is created. The results of SEDs
calculations for substars with protoplanetary disks that have a
different ages and inclinational angles are discussed.

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