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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
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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This list contains references from the content that can be linked to their source. For a full set of references and notes please see the PDF or HTML where available.

A. Ackerman & M. Marly 2001, ApJ 556, 872

F. Allard , N. F. Allard , D. Homeier 2007, A&A 474, L21

Ch. Helling , P. Woitke 2006, A&A 455, 325

H.-G. Ludwig , F. Allard , P.H. Hauschildt 2002, A&A 395, 99

D. Sudarsky , A. Burrows , I. Hubeny 2003, ApJ 588, 1121

T. Tsuji 2005, ApJ 621, 1033

P. Woitke , Ch. Helling 2004, A&A 414, 335

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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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