Spectral Variability from the Patchy Atmospheres of T and Y Dwarfs
Caroline V. Morley, Mark S. Marley, Jonathan J. Fortney, Roxana Lupu

TL;DR
This paper models spectral variability in mid-late T and Y dwarfs caused by patchy clouds and temperature perturbations, highlighting the importance of multi-wavelength observations for understanding atmospheric dynamics.
Contribution
It introduces new models for variability in T and Y dwarfs including patchy salt, sulfide, and water clouds, and explores the effects of temperature perturbations at different atmospheric levels.
Findings
Patchy cloud opacity causes significant near-infrared variability in objects over 375 K.
Water clouds increase mid-infrared variability in cooler Y dwarfs.
Temperature perturbations produce variability strongest at absorption features.
Abstract
Brown dwarfs of a variety of spectral types have been observed to be photometrically variable. Previous studies have focused on objects at the L/T transition, where the iron and silicate clouds in L dwarfs break up or dissipate. However, objects outside of this transitional effective temperature regime also exhibit variability. Here, we present models for mid-late T dwarfs and Y dwarfs. We present models that include patchy salt and sulfide clouds as well as water clouds for the Y dwarfs. We find that for objects over 375 K, patchy cloud opacity would generate the largest amplitude variability within near-infrared spectral windows. For objects under 375 K, water clouds also become important and generate larger amplitude variability in the mid-infrared. We also present models in which we perturb the temperature structure at different pressure levels of the atmosphere to simulate hot…
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