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20242026
most citedThe Sonora Substellar Atmosphere Models. IV. Elf Owl: Atmospheric Mixing and Chemical Disequilibrium with Varying Metallicity and C/O Ratios

101 citations · 104 across the 7 of their papers we have counts for

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4 papers · 1 filter

astro-ph.SR2024★ 1 cited

Protosolar D-to-H abundance and one part-per-billion PH in the coldest brown dwarf

Melanie J. Rowland, Caroline V. Morley, Brittany E. Miles +24

The coldest Y spectral type brown dwarfs are similar in mass and temperature to cool and warm (200 -- 400 K) giant exoplanets. We can therefore use their atmospheres as proxi…

astro-ph.SR2024★ 2 cited

The Sonora Substellar Atmosphere Models. III. Diamondback: Atmospheric Properties, Spectra, and Evolution for Warm Cloudy Substellar Objects

Caroline V. Morley, Sagnick Mukherjee, Mark S. Marley +7

We present a new grid of cloudy atmosphere and evolution models for substellar objects. These models include the effect of refractory cloud species, including silicate clouds, on t…

astro-ph.EP2024★ 101 cited

The Sonora Substellar Atmosphere Models. IV. Elf Owl: Atmospheric Mixing and Chemical Disequilibrium with Varying Metallicity and C/O Ratios

Sagnick Mukherjee, Jonathan J. Fortney, Caroline V. Morley +7

Disequilibrium chemistry due to vertical mixing in the atmospheres of many brown dwarfs and giant exoplanets is well-established. Atmosphere models for these objects typically para…

astro-ph.EP2024

Modeling the day-night temperature variations of ultra-hot Jupiters: confronting non-grey general circulation models and observations

Xianyu Tan, Thaddeus D. Komacek, Natasha E. Batalha +4

Ultra-hot Jupiters (UHJs) are natural laboratories to study extreme physics in planetary atmospheres and their rich observational data sets are yet to be confronted with models wit…