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Prospects of using simulations to study the photospheres of brown dwarfs
Published online by Cambridge University Press: 01 August 2006
Abstract
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We discuss prospects of using multi-dimensional time-dependent simulations to study the atmospheres of brown dwarfs and extrasolar giant planets, including the processes of convection, radiation, dust formation, and rotation. We argue that reasonably realistic simulations are feasible, however, separated into two classes of local and global models. Numerical challenges are related to potentially large dynamic ranges, and the treatment of scattering of radiation in multi-D geometries.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S239: Convection in Astrophysics , August 2006 , pp. 205 - 210
- Copyright
- Copyright © International Astronomical Union 2007
References
Allard, F., Hauschildt, P.H., Alexander, D.R., Tamanai, A. & Schweitzer, A. 2001, ApJ 556, 357CrossRefGoogle Scholar
Burkert, A., Lin, D.N.C., Bodenheimer, P.H., Jones, C.A. & Yorke, H.W. 2005, ApJ 618, 512CrossRefGoogle Scholar
Helling, Ch., 2005, in: Proceeding of he workshop on Interdisciplinary Aspects of Turbulence, Garching: Max-Planck-Institut für Astrophysik, eds.: Kupka, F., Hillebrandt, W., p. 152Google Scholar
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