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Cited article:
Ch. Helling, W.-F. Thi, P. Woitke, M. Fridlund
A&A, 451 2 (2006) L9-L12
Published online: 2006-05-02
This article has been cited by the following article(s):
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MODEL ATMOSPHERES FOR MASSIVE GAS GIANTS WITH THICK CLOUDS: APPLICATION TO THE HR 8799 PLANETS AND PREDICTIONS FOR FUTURE DETECTIONS
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Equilibrium chemistry down to 100 K
P. Woitke, Ch. Helling, G. H. Hunter, et al.
Astronomy & Astrophysics 614 A1 (2018)
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Empirically Determining Substellar Cloud Compositions in the Era of the James Webb Space Telescope
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ASpitzerInfrared Spectrograph Spectral Sequence of M, L, and T Dwarfs
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IONIZATION IN ATMOSPHERES OF BROWN DWARFS AND EXTRASOLAR PLANETS. II. DUST-INDUCED COLLISIONAL IONIZATION
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Atmospheric Parameters of Field L and T Dwarfs1
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CLOUDS IN THE COLDEST BROWN DWARFS: FIRE SPECTROSCOPY OF ROSS 458C
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WEATHER ON OTHER WORLDS. II. SURVEY RESULTS: SPOTS ARE UBIQUITOUS ON L AND T DWARFS
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The unusual protoplanetary disk around the T Tauri star ET Chamaeleontis
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The influence of dust formation modelling on Na i and K i line profiles in substellar atmospheres
C. M. S. Johnas, Ch. Helling, M. Dehn, P. Woitke and P. H. Hauschildt
Monthly Notices of the Royal Astronomical Society: Letters 385 (1) L120 (2008)
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ATMOSPHERIC CHEMISTRY IN GIANT PLANETS, BROWN DWARFS, AND LOW-MASS DWARF STARS. III. IRON, MAGNESIUM, AND SILICON
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S Lines, J Manners, N J Mayne, J Goyal, A L Carter, I A Boutle, Elspeth Lee, Ch Helling, B Drummond, D M Acreman and D K Sing
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Detection of atmospheric haze on an extrasolar planet: the 0.55-1.05 μm transmission spectrum of HD 189733b with the Hubble Space Telescope
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Consistent Simulations of Substellar Atmospheres and Nonequilibrium Dust Cloud Formation
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