Comparison of cloud models for Brown Dwarfs

Ch Helling, A. Ackerman, F. Allard, M. Dehn, P. Hauschildt, D. Homeier, K. Lodders, M. Marley, F. Rietmeijer, T. Tsuji, P. Woitke

Research output: Contribution to journalArticlepeer-review

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.

Original languageEnglish (US)
Pages (from-to)173-177
Number of pages5
JournalProceedings of the International Astronomical Union
Volume3
Issue numberS249
DOIs
StatePublished - Oct 2007
Externally publishedYes

Keywords

  • Astrochemistry
  • Brown dwarfs
  • Methods: numerical
  • Stars: atmospheres
  • Stars: low-mass

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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