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

Published online by Cambridge University Press:  10 November 2011

Olga Zakhozhay
Olga Zakhozhay*
Affiliation:
Main Astronomical Observatory National Academy of Sciences of Ukraine, 27 Akademika Zabolotnoho St. 03680 Kyiv, Ukraine email: zkholga@mail.ru
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Abstract

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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.

Keywords

circumstellar matterstars: low-massbrown dwarfsplanetary systems: protoplanetary disks
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S276: The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution , October 2010 , pp. 467 - 468
Copyright
Copyright © International Astronomical Union 2011

References

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