Limited Hysteresis in the Atmospheric Dynamics of Hot Jupiters
Over the past two decades, a coherent picture has emerged of the atmospheric dynamics of hot Jupiters from a combination of three-dimensional general circulation models and astronomical observations.
Thaddeus D. Komacek
doaj +1 more source
SIOUX project: a simultaneous multiband camera for exoplanet atmospheres studies [PDF]
Jean Marc Christille+13 more
openalex +1 more source
Revealing the atmospheres of highly irradiated exoplanets: from ultra-hot Jupiters to rocky worlds. [PDF]
Mansfield M.
europepmc +1 more source
Ground-based near-UV observations of 15 transiting exoplanets: constraints on their atmospheres and no evidence for asymmetrical transits [PDF]
Jake D. Turner+41 more
openalex +1 more source
No thick carbon dioxide atmosphere on the rocky exoplanet TRAPPIST-1 c. [PDF]
Zieba S+18 more
europepmc +1 more source
Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) [PDF]
A. Wyttenbach+15 more
openalex +1 more source
Stability of hydrides in sub-Neptune exoplanets with thick hydrogen-rich atmospheres. [PDF]
Kim T+6 more
europepmc +1 more source
Exoplanet atmospheres: a brand-new and rapidly expanding research field
Mercedes López‐Morales
openalex +2 more sources
Self-consistent atmosphere modeling with cloud formation for low-mass stars and exoplanets [PDF]
D. Juncher+2 more
openalex +1 more source
Helium in the Extended Atmosphere of the Warm Superpuff TOI-1420b
Superpuffs are planets with exceptionally low densities ( ρ ≲ 0.1 g cm ^−3 ) and core masses ( M _c ≲ 5 M _⊕ ). Many lower-mass ( M _p ≲ 10 M _⊕ ) superpuffs are expected to be unstable to catastrophic mass loss via photoevaporation and/or boil-off ...
Shreyas Vissapragada+13 more
doaj +1 more source