Results 171 to 180 of about 908,915 (272)
From Hot Jupiters to Hot Neptunes ... and Below [PDF]
M. Mayor, F. Pont, A. Vidal‐Madjar
openalex +1 more source
Age Analysis of Extrasolar Planets: Insight from Stellar Isochrone Models
There is growing evidence from stellar kinematics and galactic chemical evolution suggesting that giant planets ( M _P ≥ 0.3 M _J ) are relatively young compared to the most commonly occurring population of small planets ( M _P < 0.3 M _J ).
C. Swastik +4 more
doaj +1 more source
ELODIE metallicity-biased search for transiting Hot Jupiters [PDF]
F. Bouchy +11 more
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We present a pattern emerging from stellar obliquity measurements in single-star systems: planets with high planet-to-star mass ratios ( M _P / M _* ≥ 2 × 10 ^−3 )—such as super-Jupiters, brown dwarf companions, and M dwarfs hosting Jupiter-like planets ...
Jace Rusznak +3 more
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Planet population synthesis: the role of stellar encounters. [PDF]
Ndugu N, Abedigamba OP, Andama G.
europepmc +1 more source
Formation of Ultra-short-period Planets in Hot Jupiter Systems: Application to WASP-47
The WASP-47 system is notable as the first known system hosting both inner and outer low-mass planetary companions around a hot Jupiter, with an ultra-short-period (USP) planet as the innermost planetary companion.
Su Wang +4 more
doaj +1 more source
An Eccentric Hot Jupiter Orbiting the Subgiant HD 185269 [PDF]
John Asher Johnson +6 more
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Giant planets are expected to predominantly form beyond the water-ice line and occasionally undergo inward migration. Unlike hot Jupiters, which can result from high-eccentricity tidal migration, warm Jupiters between 0.1 and 1 au (≈10–365 days) are in ...
Marvin Morgan +6 more
doaj +1 more source
Upper limits on the hot Jupiter fraction in the field of NGC 7789 [PDF]
D. M. Bramich, K. Horne
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A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b. [PDF]
Coulombe LP +75 more
europepmc +1 more source

