Results 81 to 90 of about 2,846 (170)

Planet population synthesis: the role of stellar encounters. [PDF]

open access: yesMon Not R Astron Soc, 2022
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

open access: yesThe Planetary Science Journal
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

open access: yesThe Astronomical Journal
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]

open access: green, 2016
Giovanni Rosotti   +5 more
openalex   +1 more source

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest Mp/M* Systems Exhibit Low Obliquities, Even around Hot Stars

open access: yesThe Astrophysical Journal Letters
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]

open access: yesNature, 2023
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]

open access: green, 2018
C. von Essen   +6 more
openalex   +1 more source

Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters

open access: yesThe Astrophysical Journal Supplement Series
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]

open access: bronze, 2021
D. Cont   +24 more
openalex   +1 more source

A survey of eight hot Jupiters in secondary eclipse using WIRCam at CFHT. [PDF]

open access: yesMon Not R Astron Soc, 2018
Martioli E   +14 more
europepmc   +1 more source

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