Photochemically produced SO2 in the atmosphere of WASP-39b
Photochemistry is a fundamental process of planetary atmospheres that regulates the
atmospheric composition and stability. However, no unambiguous photochemical products …
atmospheric composition and stability. However, no unambiguous photochemical products …
[HTML][HTML] The 2024 release of the ExoMol database: Molecular line lists for exoplanet and other hot atmospheres
The ExoMol database (www. exomol. com) provides molecular data for spectroscopic
studies of hot atmospheres. These data are widely used to model atmospheres of …
studies of hot atmospheres. These data are widely used to model atmospheres of …
A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b
LP Coulombe, B Benneke, R Challener, AAA Piette… - Nature, 2023 - nature.com
Close-in giant exoplanets with temperatures greater than 2,000 K ('ultra-hot Jupiters') have
been the subject of extensive efforts to determine their atmospheric properties using thermal …
been the subject of extensive efforts to determine their atmospheric properties using thermal …
PICASO 3.0: a one-dimensional climate model for giant planets and brown dwarfs
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 …
exoplanet and brown dwarf atmospheres in great detail. The physical interpretation of these …
Probing the extent of vertical mixing in brown dwarf atmospheres with disequilibrium chemistry
Evidence of disequilibrium chemistry due to vertical mixing in the atmospheres of many T-
and Y-dwarfs has been inferred due to enhanced mixing ratios of CO and reduced NH 3 …
and Y-dwarfs has been inferred due to enhanced mixing ratios of CO and reduced NH 3 …
Exploring the effects of active magnetic drag in a general circulation model of the ultrahot Jupiter WASP-76b
Ultrahot Jupiters represent an exciting avenue for testing extreme physics and observing
atmospheric circulation regimes not found in our solar system. Their high temperatures …
atmospheric circulation regimes not found in our solar system. Their high temperatures …
[HTML][HTML] Patchy nightside clouds on ultra-hot Jupiters: general circulation model simulations with radiatively active cloud tracers
The atmospheres of ultra-hot Jupiters have been characterized in detail through recent
phase curve and low-and high-resolution emission and transmission spectroscopic …
phase curve and low-and high-resolution emission and transmission spectroscopic …
Modelling dynamically driven global cloud formation microphysics in the HAT-P-1b atmosphere
EKH Lee - Monthly Notices of the Royal Astronomical Society, 2023 - academic.oup.com
Insight into the formation and global distribution of cloud particles in exoplanet atmospheres
continues to be a key problem to tackle going into the JWST era. Understanding …
continues to be a key problem to tackle going into the JWST era. Understanding …
No umbrella needed: Confronting the hypothesis of iron rain on WASP-76b with post-processed general circulation models
AB Savel, EMR Kempton, M Malik… - The Astrophysical …, 2022 - iopscience.iop.org
High-resolution spectra are unique indicators of three-dimensional (3D) processes in
exoplanetary atmospheres. For instance, in 2020, Ehrenreich et al. reported transmission …
exoplanetary atmospheres. For instance, in 2020, Ehrenreich et al. reported transmission …
Exploring the deep atmospheres of HD 209458b and WASP-43b using a non-gray general circulation model
AD Schneider, L Carone, L Decin… - Astronomy & …, 2022 - aanda.org
Simulations with a 3D general circulation model (GCM) suggest that one potential driver
behind the observed radius inflation in hot Jupiters may be the downward advection of …
behind the observed radius inflation in hot Jupiters may be the downward advection of …