We provide a brief review of many aspects of the planetary physics of hot Jupiters. Our aim is
to cover most of the major areas of current study while providing the reader with additional …

Groundbased and spacecraft telescopic observations, combined with an intensive modeling
effort, have greatly enhanced our understanding of hot giant planets and brown dwarfs over …

Population studies of exoplanets are key to unlocking their statistical properties. So far, the
inferred properties have been mostly limited to planetary, orbital, and stellar parameters …

We present an update of the open-source photochemical kinetics code VULCAN to include
C–H–N–O–S networks and photochemistry. The additional new features are advection …

Ground-based high-resolution spectroscopy (HRS) has detected numerous chemical
species and atmospheric dynamics in exoplanets, most notably ultrahot Jupiters (UHJs) …

Hot Jupiters have been predicted to have a strong day/night temperature contrast and a
hotspot shifted eastward of the substellar point. This was confirmed by numerous phase …

Ultra-hot Jupiters are tidally locked gas giants with dayside temperatures high enough to
dissociate hydrogen and other molecules. Their atmospheres are vastly non-uniform in …

Hydrogen at extreme temperatures and pressures is of key relevance for cutting-edge
technological applications, with inertial confinement fusion research being a prime example …

Ultrahot Jupiters represent an exciting avenue for testing extreme physics and observing
atmospheric circulation regimes not found in our solar system. Their high temperatures …

Exoplanet atmospheres are inherently three-dimensional systems in which thermal/chemical
variation and winds can strongly influence spectra. Recently, the ultra-hot Jupiter WASP-76 …