Global flow regimes of hot Jupiters
Context: the atmospheric dynamics of hot and ultrahot Jupiters are influenced by the stellar irradiation they receive, which shapes their atmospheric circulation and the underlying wave structures.
Heng, K. +4 more
core +1 more source
CHES: An astrometry mission searching for nearby habitable planets. [PDF]
Ji J, Wang S, Li H, Fang L, Li D.
europepmc +1 more source
CHEMICAL CONSEQUENCES OF THE C/O RATIO ON HOT JUPITERS: EXAMPLES FROM WASP-12b, COROT-2b, XO-1b, AND HD 189733b. [PDF]
Moses JI +3 more
europepmc +1 more source
Stellar clustering shapes the architecture of planetary systems. [PDF]
Winter AJ +3 more
europepmc +1 more source
Radio Emission from Red-Giant Hot Jupiters
When planet-hosting stars evolve off the main sequence and go through the red-giant branch, the stars become orders of magnitudes more luminous and, at the same time, lose mass at much higher rates than their main sequence counterparts.
Mroczkowski, Tony +7 more
core
The rotational and divergent components of atmospheric circulation on tidally locked planets. [PDF]
Hammond M, Lewis NT.
europepmc +1 more source
Exploring exoplanet dynamics with JWST: Tides, rotation, rings, and moons. [PDF]
Millholland SC, Winn JN.
europepmc +1 more source
Atmospheric composition of exoplanets based on the thermal escape of gases and implications for habitability. [PDF]
Konatham S, Martin-Torres J, Zorzano MP.
europepmc +1 more source
A Stellar magnesium to silicon ratio in the atmosphere of an exoplanet. [PDF]
Sanchez JA +19 more
europepmc +1 more source
A Synchronized Two-Dimensional α-Ω Model of the Solar Dynamo. [PDF]
Klevs M, Stefani F, Jouve L.
europepmc +1 more source

