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Dependence of Circumsubstellar Disk SEDs on System Inclination

Published online by Cambridge University Press:  23 April 2012

Olga Zakhozhay*
Affiliation:
Main Astronomical Observatory, National Academy of Sciences of Ukraine, 27, Akad. Zabolotny St., Kyiv, 03680, Ukraine email: [email protected]
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

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