Measuring and Replicating the 1–20 μm Energy Distributions of the Coldest Brown Dwarfs: Rotating, Turbulent, and Nonadiabatic Atmospheres

Cold, low-mass, field brown dwarfs are important for constraining the terminus of the stellar mass function, and also for optimizing atmospheric studies of exoplanets. In 2020 new model grids for such objects were made available: Sonora-Bobcat and ATMO 2020. Also, new candidate cold brown dwarfs wer...

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Veröffentlicht in:	The Astrophysical journal Jg. 918; H. 1; S. 11 - 41
Hauptverfasser:	Leggett, S. K., Tremblin, Pascal, Phillips, Mark W., Dupuy, Trent J., Marley, Mark, Morley, Caroline, Schneider, Adam, Caselden, Dan, Guillaume, Colin, Logsdon, Sarah E.
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	Philadelphia The American Astronomical Society 01.09.2021 IOP Publishing
Schlagworte:	Ammonia Astrophysics Atmosphere Atmospheric models Atmospheric pressure Brown dwarf stars Brown dwarfs Energy distribution Extrasolar planets Infrared photometry Infrared sources Photometry Photosphere Rotation Stellar atmospheres Stellar convective zones Stellar mass Temperature gradients Temperature profiles Yttrium
ISSN:	0004-637X, 1538-4357
Online-Zugang:	Volltext
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