[HTML][HTML] Atmospheric dynamics of hot giant planets and brown dwarfs

AP Showman, X Tan, V Parmentier - Space Science Reviews, 2020 - Springer
Groundbased and spacecraft telescopic observations, combined with an intensive modeling
effort, have greatly enhanced our understanding of hot giant planets and brown dwarfs over …

On the cool side: modeling the atmospheres of brown dwarfs and giant planets

MS Marley, TD Robinson - Annual Review of Astronomy and …, 2015 - annualreviews.org
The atmosphere of a brown dwarf or extrasolar giant planet controls the spectrum of
radiation emitted by the object and regulates its cooling over time. Although the study of …

Gaia Data Release 3-Astrophysical parameters inference system (Apsis). I. Methods and content overview

OL Creevey, R Sordo, F Pailler, Y Frémat… - Astronomy & …, 2023 - aanda.org
Gaia Data Release 3 contains a wealth of new data products for the community.
Astrophysical parameters are a major component of this release, and were produced by the …

The Sonora brown dwarf atmosphere and evolution models. I. Model description and application to cloudless atmospheres in rainout chemical equilibrium

MS Marley, D Saumon, C Visscher… - The Astrophysical …, 2021 - iopscience.iop.org
We present a new generation of substellar atmosphere and evolution models, appropriate
for application to studies of L-, T-, and Y-type brown dwarfs and self-luminous extrasolar …

[HTML][HTML] Gaia Data Release 3-Apsis. II. Stellar parameters

M Fouesneau, Y Frémat, R Andrae, AJ Korn… - Astronomy & …, 2023 - aanda.org
Context. The third Gaia data release (Gaia DR3) contains, beyond the astrometry and
photometry, dispersed light for hundreds of millions of sources from the Gaia prism spectra …

A new set of atmosphere and evolution models for cool T–Y brown dwarfs and giant exoplanets

MW Phillips, P Tremblin, I Baraffe, G Chabrier… - Astronomy & …, 2020 - aanda.org
We present a new set of solar metallicity atmosphere and evolutionary models for very cool
brown dwarfs and self-luminous giant exoplanets, which we term ATMO 2020. Atmosphere …

Aerosol composition of hot giant exoplanets dominated by silicates and hydrocarbon hazes

P Gao, DP Thorngren, EKH Lee, JJ Fortney… - Nature …, 2020 - nature.com
Aerosols are common in the atmospheres of exoplanets across a wide swath of
temperatures, masses and ages,–. These aerosols strongly impact observations of …

Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager

B Macintosh, JR Graham, T Barman, RJ De Rosa… - Science, 2015 - science.org
Directly detecting thermal emission from young extrasolar planets allows measurement of
their atmospheric compositions and luminosities, which are influenced by their formation …

Fundamental parameters and spectral energy distributions of young and field age objects with masses spanning the stellar to planetary regime

JC Filippazzo, EL Rice, J Faherty, KL Cruz… - The Astrophysical …, 2015 - iopscience.iop.org
We combine optical, near-infrared, and mid-infrared spectra and photometry to construct
expanded spectral energy distributions for 145 field age (> 500 Myr) and 53 young (lower …

PICASO 3.0: a one-dimensional climate model for giant planets and brown dwarfs

S Mukherjee, NE Batalha, JJ Fortney… - The Astrophysical …, 2023 - iopscience.iop.org
Abstract Upcoming James Webb Space Telescope observations will allow us to study
exoplanet and brown dwarf atmospheres in great detail. The physical interpretation of these …