Clouds and Clearings in the Atmospheres of the L and T Dwarfs

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dc.creatorMarley, M. S.
dc.creatorAckerman, A.
dc.creatorBurgasser, A. J.
dc.creatorSaumon, D.
dc.creatorLodders, K.
dc.creatorFreedman, R.
dc.date2002-07-31
dc.date.accessioned2026-07-07T02:04:30Z
dc.date.available2026-07-07T02:04:30Z
dc.descriptionA sophisticated approach to condensate opacity is required to properly model the atmospheres of L and T dwarfs. Here we review different models for the treatment of condensates in brown dwarf atmospheres. We conclude that models which include both particle sedimentation and upwards transport of condensate (both gas and particles) provide the best fit for the L dwarf colors. While a globally uniform cloud model fits the L dwarf data, it turns to the blue in J-K too slowly to fit the T dwarfs. Models which include local clearings in the global cloud deck, similar to Jupiter's prominent five-micron hot spots, better reproduce the available photometric data and also account for the observed resurgence of FeH absorption in early type T dwarfs.
dc.description12 pages, 2 figures, in newpasp.sty format, To appear in "IAU Symposium 211: Brown Dwarfs", E.L. Martin Ed., Publications of the Astronomical Society of the Pacific, Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0207658
dc.identifierhttp://arxiv.org/abs/astro-ph/0207658
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4781
dc.subjectAstrophysics
dc.titleClouds and Clearings in the Atmospheres of the L and T Dwarfs
dc.typetext

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