Results 111 to 120 of about 624,657 (195)
Towards Doppler eclipse mapping of hot Jupiters
Context. In the last decade, ground-based high-resolution spectroscopy (HRS) has emerged as a powerful method to probe exoplanet atmospheres both in transit and thermal emission.
Yariv V. +9 more
doaj +1 more source
Warm Jupiters with orbital periods of ≈10–365 days represent a population of giant planets located well within the water ice line but beyond the region of tidal influence of their host star relevant for high-eccentricity tidal migration.
Marvin Morgan +2 more
doaj +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
Planet population synthesis: the role of stellar encounters. [PDF]
Ndugu N, Abedigamba OP, Andama G.
europepmc +1 more source
The Nitrogen Chemistry in Hot Jupiters Atmosphere
International audienceThe atmosphere of hot Jupiters can be probed by primary transit and secondary eclipse spectroscopy. In order to constrain the atmospheric thermal structure and composition from observables, chemical models are necessary.
Eric Hébrard +19 more
core +1 more source
The ExoEcho project is designed to study the photodynamics of exoplanets by leveraging high-precision transit timing data from ground- and space-based telescopes.
Xinyue Ma +8 more
doaj +1 more source
LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements. [PDF]
Dong S, Xie JW, Zhou JL, Zheng Z, Luo A.
europepmc +1 more source
Stability of Multiplanet Systems through Hot Jupiter Destruction
Recent observational and theoretical work suggests that the sub-Jovian desert (periods ≲3 days, masses ∼10–100 M _⊕ ) hosts the remains of destroyed hot Jupiters (“desert dwellers”).
Donald Liveoak +2 more
doaj +1 more source
“Popcorn Planets” Are Not Actively Inflated by Eccentricity Tides
Recent discoveries have revealed a population of “popcorn planets” that have masses similar to that of Neptune but radii comparable to Jupiter, leading to exceptionally low bulk densities ρ _p ≲ 0.3 g cm ^−3 .
Samuel W. Yee, Shreyas Vissapragada
doaj +1 more source
Secular chaos and its application to Mercury, hot Jupiters, and the organization of planetary systems. [PDF]
Lithwick Y, Wu Y.
europepmc +1 more source

