High-eccentricity Migration with Disk-induced Spin–Orbit Misalignment: A Preference for Perpendicular Hot Jupiters [PDF]
Astrophysical Journal Letters, 2022 High-eccentricity migration is a likely formation mechanism for many observed hot Jupiters, particularly those with a large misalignment between the stellar spin axis and orbital angular momentum axis of the planet.
M. Vick, Yubo Su, D. Lai
semanticscholar +1 more source
H2S and SO2 detectability in hot Jupiters. Sulphur species as indicators of metallicity and C/O ratio [PDF]
Astronomy & Astrophysics, 2022 The high cosmic abundance and the intermediate volatility and chemical properties of sulfur allow the use of sulfur-bearing species as a tracer of the chemical processes in the atmospheres of hot Jupiter exoplanets.
J. Polman +4 more
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The Effect of Interior Heat Flux on the Atmospheric Circulation of Hot and Ultra-hot Jupiters [PDF]
Astrophysical Journal Letters, 2022 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 that impinges upon the atmosphere from below.
T. Komacek +4 more
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HOT STARS WITH HOT JUPITERS HAVE HIGH OBLIQUITIES [PDF]
The Astrophysical Journal, 2010 ApJ Letters, in press [6 pages]
Joshua N. Winn +3 more
openalex +9 more sources
HOT JUPITER MAGNETOSPHERES [PDF]
The Astrophysical Journal, 2011 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 ...
Phil Arras +2 more
openaire +3 more sources
A Uniform Search for Nearby Planetary Companions to Hot Jupiters in TESS Data Reveals Hot Jupiters Are Still Lonely [PDF]
Astronomical Journal, 2021 We present the results of a uniform search for additional planets around all stars with confirmed hot Jupiters observed by the Transiting Exoplanet Survey Satellite (TESS) in its Cycle 1 survey of the southern ecliptic hemisphere.
B. Hord +14 more
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Hot Jupiters: Origins, Structure, Atmospheres [PDF]
Journal of Geophysical Research: Planets, 2021 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 references for more detailed follow‐up.
J. Fortney, R. Dawson, T. Komacek
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A Universal Cloud Composition on the Nightsides of Hot Jupiters [PDF]
Astrophysical Journal Letters, 2021 The day and nightside temperatures of hot Jupiters are diagnostics of heat transport processes in their atmospheres. Recent observations have shown that the nightsides of hot Jupiters are a nearly constant 1100 K for a wide range of equilibrium ...
P. Gao, D. Powell
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HOT JUPITERS AND COOL STARS [PDF]
The Astrophysical Journal, 2014 38 pages, 15 figures, accepted for publication in ...
Lionel Siess +4 more
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Slow Cooling and Fast Reinflation for Hot Jupiters [PDF]
, 2021 The unexpectedly large radii of hot Jupiters are a longstanding mystery whose solution will provide important insights into their interior physics.
D. Thorngren +4 more
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