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Dependence of Circumsubstellar Disk SEDs on System Inclination

Published online by Cambridge University Press:  23 April 2012

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

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The spectral energy distributions (SEDs) have being simulated for 1120 systems that contain brown dwarfs with different physical parameters and protoplanetary disks that are inclined at different angles. The SED's shape dependence on disk inclination toward the observer is discussed.

Keywords

circumstellar matterstars: low-massbrown dwarfsplanetary systems: protoplanetary disks

References

Pisarenko, I. A., Yatsenko, A. A., & Zakhozhay, V. A. 2007, Astron. Rep., 51, 605CrossRefGoogle Scholar
Chiang, E. I. & Goldreich, P. 1997, ApJ, 490, 368CrossRefGoogle Scholar
Zakhozhay, O. V. 2011, Radio Physics and Radio Astronomy, 2, 125CrossRefGoogle Scholar
Zakhozhay, O. V. 2011, Radio Physics and Radio Astronomy, 2, 211CrossRefGoogle Scholar
Zakhozhay, V. A., Zakhozhay, O. V., & Vidmachenko, A. P. 2011, Kin. Phys. Cel. Bodies, 27, 140CrossRefGoogle Scholar
Zakhozhay, O. V. 2005, Vysnyk astronomichnoi shkoly (in Russian), 4, 55Google Scholar