Results 81 to 90 of about 2,846 (170)
Planet population synthesis: the role of stellar encounters. [PDF]
Ndugu N, Abedigamba OP, Andama G.
europepmc +1 more source
Orbital Decay Candidates Reconsidered: WASP-4 b Is Not Decaying and Kepler-1658 b Is Not a Planet
The fate of hot Jupiters is thought to be engulfment by their host stars, the outcome of tidal orbital decay. Transit timing has revealed a few systems with apparently shrinking orbital periods, but such signals can be mimicked by light travel-time ...
Joshua N. Winn, Guđmundur Stefánsson
doaj +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
The origin of the eccentricity of the hot Jupiter in CI Tau [PDF]
Giovanni Rosotti +5 more
openalex +1 more source
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
doaj +1 more source
A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b. [PDF]
Coulombe LP +75 more
europepmc +1 more source
An optical transmission spectrum of the ultra-hot Jupiter WASP-33b. First indication of AlO in an exoplanet [PDF]
C. von Essen +6 more
openalex +1 more source
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
Silicon in the dayside atmospheres of two ultra-hot Jupiters [PDF]
D. Cont +24 more
openalex +1 more source
A survey of eight hot Jupiters in secondary eclipse using WIRCam at CFHT. [PDF]
Martioli E +14 more
europepmc +1 more source

