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Comparison of cloud models for Brown Dwarfs

  • Ch. Helling (a1), A. Ackerman (a2), F. Allard (a3), M. Dehn (a4), P. Hauschildt (a4), D. Homeier (a5), K. Lodders (a6), M. Marley (a7), F. Rietmeijer (a8), T. Tsuji (a9) and P. Woitke (a10)...
Abstract

A test case comparison is presented for different dust cloud model approaches applied in brown dwarfs and giant gas planets. We aim to achieve more transparency in evaluating the uncertainty inherent to theoretical modelling. We show in how far model results for characteristic dust quantities vary due to different assumptions. We also demonstrate differences in the spectral energy distributions resulting from our individual cloud modelling in 1D substellar atmosphere simulations.

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References
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Ackerman, A. & Marly, M. 2001, ApJ 556, 872
Allard, F., Allard, N. F., Homeier, D. et al. 2007, A&A 474, L21
Allard, F., Guillot, T., Ludwig, H.-G., Hauschildt, P. H., et al. 2003, IAU 211, 325
Dehn, M. 2007, PhD Thesis, University Hamburg
Helling, Ch., Woitke, P., Thi, W.-F. 2008, submitted
Helling, Ch., Woitke, P. 2006, A&A 455, 325
Ludwig, H.-G., Allard, F., Hauschildt, P.H. 2002, A&A 395, 99
Sudarsky, D., Burrows, A., Hubeny, I. 2003, ApJ 588, 1121
Tsuji, T. 2005, ApJ 621, 1033
Woitke, P., Helling, Ch. 2004, A&A 414, 335
Woitke, P., Helling, Ch. 2003, A&A 388, 297
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Proceedings of the International Astronomical Union
  • ISSN: 1743-9213
  • EISSN: 1743-9221
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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