[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 …
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 …
Diagnosing limb asymmetries in hot and ultrahot Jupiters with high-resolution transmission spectroscopy
AB Savel, EMR Kempton, E Rauscher… - The Astrophysical …, 2023 - iopscience.iop.org
Due to their likely tidally synchronized nature,(ultra) hot Jupiter atmospheres should
experience strongly spatially heterogeneous instellation. The large irradiation contrast and …
experience strongly spatially heterogeneous instellation. The large irradiation contrast and …
The effect of interior heat flux on the atmospheric circulation of hot and ultra-hot Jupiters
Many hot and ultra-hot Jupiters have inflated radii, implying that their interiors retain
significant entropy from formation. These hot interiors lead to an enhanced internal heat flux …
significant entropy from formation. These hot interiors lead to an enhanced internal heat flux …
Avoiding a cluster catastrophe: Retention efficiency and the binary black hole mass spectrum
The population of binary black hole mergers identified through gravitational waves has
uncovered unexpected features in the intrinsic properties of black holes in the universe. One …
uncovered unexpected features in the intrinsic properties of black holes in the universe. One …
Coupling haze and cloud microphysics in WASP-39b's atmosphere based on JWST observations
A Arfaux, P Lavvas - Monthly Notices of the Royal Astronomical …, 2024 - academic.oup.com
We present a study on the coupling of haze and clouds in the atmosphere of WASP-39b. We
developed a cloud microphysics model simulating the formation of Na2S and MgSiO3 …
developed a cloud microphysics model simulating the formation of Na2S and MgSiO3 …
The radiative and dynamical impact of clouds in the atmosphere of the hot Jupiter WASP-43 b
Context. Hot Jupiters are tidally locked gaseous exoplanets that exhibit large day-night
temperature contrasts. Their cooler nightsides are thought to host clouds, as has been …
temperature contrasts. Their cooler nightsides are thought to host clouds, as has been …
Dimming the Lights: 2D Simulations of Deflagrations of Hybrid C/O/Ne White Dwarfs Using FLASH
C Feldman, N Gutierrez, E Eisenberg… - The Astrophysical …, 2023 - iopscience.iop.org
The dimmest and most numerous outlier of the Type Ia supernova population, the Type Iax
event, is increasingly being found in the results of observational campaigns. There is …
event, is increasingly being found in the results of observational campaigns. There is …
Temporal albedo variability in the phase curve of KELT-1b
H Parviainen - Astronomy & Astrophysics, 2023 - aanda.org
The dayside brightness spectrum of a highly irradiated transiting brown dwarf KELT-1b is
challenging to explain based on current brown dwarf atmosphere models. The spectrum has …
challenging to explain based on current brown dwarf atmosphere models. The spectrum has …
MOA-2020-BLG-208Lb: cool sub-Saturn-mass planet within predicted desert
MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert - IOPscience
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