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Astrophysics

arXiv:0711.3993 (astro-ph)
[Submitted on 26 Nov 2007]

Title:Comparison of cloud models for Brown Dwarfs

Authors:Ch.Helling, A.Ackerman, F.Allard, M.Dehn, P.Hauschildt, D.Homeier, K.Lodders, M.Marley, F.Rietmeijer, T.Tsuji, P.Woitke
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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
Comments: 5 pages, Proceeding to "Exoplantes: Detection, Formation, Dynamics", eds. Ferraz-Mello et a
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:0711.3993 [astro-ph]
  (or arXiv:0711.3993v1 [astro-ph] for this version)
  https://doi.org/10.48550/arXiv.0711.3993
Related DOI: https://doi.org/10.1017/S1743921308016578

Submission history

From: Christiane Helling [view email]
[v1] Mon, 26 Nov 2007 13:02:07 UTC (169 KB)
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