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 language | English (US) |
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Pages (from-to) | 173-177 |
Number of pages | 5 |
Journal | Proceedings of the International Astronomical Union |
Volume | 3 |
Issue number | S249 |
DOIs | |
State | Published - Oct 2007 |
Externally published | Yes |
Keywords
- Astrochemistry
- Brown dwarfs
- Methods: numerical
- Stars: atmospheres
- Stars: low-mass
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science