Results 1 to 10 of about 449 (146)
Hot Jupiters Are Asynchronous Rotators
Hot Jupiters are typically assumed to be synchronously rotating, from tidal locking. Their thermally driven atmospheric winds experience Lorentz drag on the planetary magnetic field anchored at depth.
Marek Wazny, Kristen Menou
doaj +3 more sources
Evaporation of hot jupiters and hot neptunes [PDF]
Among the nearly five hundred extra-solar planets known, almost 30% orbit closer than 0.1 AU from their parent star. We will review the observations and the corresponding models of the evaporation of these ‘hot jupiters’.
Ehrenreich D.
doaj +2 more sources
The WFCAM Transit Survey (WTS) is a near-infrared transit survey running on the United Kingdom Infrared Telescope (UKIRT). We conduct Monte Carlo transit injection and detection simulations for short period (
Murgas F. +13 more
doaj +2 more sources
Hot Jupiters from Disruption of Resonant Chains in Postdisk Evolution
The formation of hot Jupiters has been a subject of interest in the field of exoplanet science. According to conventional scenarios, these gas giants are believed to form beyond the snow line and subsequently migrate inward.
Dong-Hong Wu, Ying He
doaj +1 more source
HOT JUPITER MAGNETOSPHERES [PDF]
26 pages, 17 figures (5 color), 2 appendices; submitted to ApJ; higher resolution version available at http://www.astro.virginia.edu/~gbt8f/HotJupMag_fullres_astroph ...
Trammell, George B. +2 more
openaire +2 more sources
Statistical Analysis of the Dearth of Super-eccentric Jupiters in the Kepler Sample
Hot Jupiters may have formed in situ, or been delivered to their observed short periods through one of two categories of migration mechanisms: disk migration or high-eccentricity migration.
Jonathan M. Jackson +3 more
doaj +1 more source
Evidence for Hidden Nearby Companions to Hot Jupiters
The first discovered extrasolar worlds—giant, “hot Jupiter” planets on short-period orbits—came as a surprise to solar system–centric models of planet formation, prompting the development of new theories for planetary system evolution.
Dong-Hong Wu, Malena Rice, Songhu Wang
doaj +1 more source
Atmospheric circulation of exoplanets
To date, more than 5000 exoplanets and more than 2000 brown dwarfs have been confirmed, which shows rich diversities in many aspects. With the rapid growth of the planet family, both observational and theoretical research on exoplanet atmosphere is ...
Yuchen Lian, Yongyun Hu
doaj +1 more source
HOT JUPITERS AND COOL STARS [PDF]
38 pages, 15 figures, accepted for publication in ...
Villaver, Eva +3 more
openaire +3 more sources
ATMOSPHERIC ESCAPE FROM HOT JUPITERS [PDF]
Accepted for publication in ApJ, 22 pages, 24 figures. Added additional references--in particular, we now discuss charge-exchange as a potential source of high-velocity ...
Murray-Clay, Ruth +2 more
openaire +2 more sources

