Results 21 to 30 of about 624,657 (195)
Colour–colour and colour–magnitude diagrams for hot Jupiters [PDF]
, 2020 We use ground-based and space-based eclipse measurements for the near-infrared (IR) bands (JHKs) and Spitzer 3.6- and 4.5-μm bands to construct colour–colour and colour–magnitude diagrams for hot Jupiters.
Melville, G. +2 more
core +1 more source
HOT JUPITERS AND COOL STARS [PDF]
The Astrophysical Journal, 2014 38 pages, 15 figures, accepted for publication in ...
Villaver, Eva +3 more
openaire +3 more sources
CIRCULATION AND DISSIPATION ON HOT JUPITERS [PDF]
The Astrophysical Journal, 2010 Many global circulation models predict supersonic zonal winds and large vertical shears in the atmospheres of short-period jovian exoplanets. Using linear analysis and nonlinear local simulations, we investigate hydrodynamic dissipation mechanisms to balance the thermal acceleration of these winds.
Li, Jason, Goodman, Jeremy
openaire +2 more sources
Hot-Jupiters and hot-Neptunes: A common origin? [PDF]
Astronomy & Astrophysics, 2005 5 pages, 2 figures, accepted in A&A ...
Baraffe, I. +5 more
openaire +2 more sources
Inflation of migrated hot Jupiters
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT The observed low densities of gas giant planets with a high equilibrium temperature (hot Jupiters) can be simulated in models when a fraction of the surface radiation is deposited deeper in the interior. Meanwhile, migration theories suggest that hot Jupiters formed further away from their host star and migrated inward.
Mol Lous, M.A.S., Miguel, Y.
openaire +4 more sources
INFLATING HOT JUPITERS WITH OHMIC DISSIPATION [PDF]
The Astrophysical Journal, 2010 We present a new, magnetohydrodynamic mechanism for inflation of close-in giant extrasolar planets. The idea behind the mechanism is that current, which is induced through interaction of atmospheric winds and the planetary magnetic field, results in significant Ohmic dissipation of energy in the interior.
Batygin, Konstantin, Stevenson, David J.
openaire +3 more sources
New Clues to Reveal Origins of Hot- and Warm-Jupiter: Mutual Occurrence Rate of Hot Jupiter，Warm Jupiter and Cold Jupiter [PDF]
, 2021 Abstract Many works based on the correlations between the occurrence rate of various giant planets and stellar properties of their hosts have provided clues revealing planetary formation processes. However, few researches have focused on the mutual occurrence rate of different type of planets and their dependency upon the stellar properties ...
Xiangning Su, Hui Zhang, Jilin Zhou
openaire +1 more source
Evidence of three mechanisms explaining the radius anomaly of hot Jupiters [PDF]
, 2021 Context. The anomalously large radii of hot Jupiters are still not fully understood, and all of the proposed explanations are based on the idea that these close-in giant planets possess hot interiors. Most of the mechanisms proposed have been tested on a
P. Mollière +9 more
core +3 more sources
Photochemical haze, a common aerosol type expected to form in the atmospheres of hot-Jupiters, can become concentrated to different extents between the morning and evening limbs depending on the balance between advection, gravitational settling, and ...
David K Sing (14714917) +3 more
core +6 more sources
Magnetohydrodynamics in hot Jupiters [PDF]
, 2021 PhD ThesisHot Jupiters are Jupiter-like exoplanets found in close-in orbits. This subjects them to high levels of stellar irradiance and is believed to tidally-lock them to their host stars, causing extreme day-night temperature differentials which in ...
Hindle, Alexander William
core +1 more source