%0 Journal Article %1 Saumon2000 %A Saumon, D. %A Geballe, T. R. %A Leggett, S. K. %A Marley, M. S. %A Freedman, R. S. %A Lodders, K. %A Fegley, B. %A Sengupta, S. K. %D 2000 %J ASTROPHYSICAL JOURNAL %K 229B; BROWN CARBON-MONOXIDE; CHEMISTRY; COOL DISCOVERY; DWARF; GIANT GLIESE JUPITER; METHANE; MODELS PLANETS; SPECTRUM; %N 1 %P 374--389 %T Molecular abundances in the atmosphere of the T dwarf G1 229B %V 541 %X We present new high-resolution infrared spectra of the T dwarf Gliese 229B in the J, H, and K bandpasses. We analyze each of these as well as previously published spectra to determine its metallicity and the abundances of NH, and CO in terms of the surface gravity of G1 229B, which remains poorly constrained. The metallicity increases with increasing gravity and is below the solar value unless G1 229B is a high-gravity brown dwarf with log g (cgs) approximate to 5.5. The NH3 abundance is determined from both the Hand the K-band spectra, which probe two different levels in the atmosphere. We find that the abundance from the K-band data is well below that expected from chemical equilibrium, which we interpret as strong evidence for dynamical transport of NH3 in the atmosphere. This is consistent with the previous detection of CO and provides additional constraints on the dynamics of the atmosphere of this T dwarf.

@article{Saumon2000, abstract = {We present new high-resolution infrared spectra of the T dwarf Gliese 229B in the J, H, and K bandpasses. We analyze each of these as well as previously published spectra to determine its metallicity and the abundances of NH, and CO in terms of the surface gravity of G1 229B, which remains poorly constrained. The metallicity increases with increasing gravity and is below the solar value unless G1 229B is a high-gravity brown dwarf with log g (cgs) approximate to 5.5. The NH3 abundance is determined from both the Hand the K-band spectra, which probe two different levels in the atmosphere. We find that the abundance from the K-band data is well below that expected from chemical equilibrium, which we interpret as strong evidence for dynamical transport of NH3 in the atmosphere. This is consistent with the previous detection of CO and provides additional constraints on the dynamics of the atmosphere of this T dwarf.}, added-at = {2009-11-03T20:21:25.000+0100}, author = {Saumon, D. and Geballe, T. R. and Leggett, S. K. and Marley, M. S. and Freedman, R. S. and Lodders, K. and Fegley, B. and Sengupta, S. K.}, biburl = {https://www.bibsonomy.org/bibtex/24b83e5c0cdb34076318e14acc683a0e0/svance}, interhash = {fa86691014a3f2d034ed0c825e9b5445}, intrahash = {4b83e5c0cdb34076318e14acc683a0e0}, journal = {ASTROPHYSICAL JOURNAL}, keywords = {229B; BROWN CARBON-MONOXIDE; CHEMISTRY; COOL DISCOVERY; DWARF; GIANT GLIESE JUPITER; METHANE; MODELS PLANETS; SPECTRUM;}, number = 1, owner = {svance}, pages = {374--389}, timestamp = {2009-11-03T20:22:13.000+0100}, title = {Molecular abundances in the atmosphere of the T dwarf G1 229B}, volume = 541, year = 2000 }