Results 131 to 140 of about 22,266,209 (231)

Detecting ring systems around exoplanets using high resolution spectroscopy: the case of 51 Pegasi b [PDF]

open access: bronze, 2015
N. C. Santos   +15 more
openalex   +1 more source

FIVE NEW EXOPLANETS ORBITING THREE METAL-RICH, MASSIVE STARS: TWO-PLANET SYSTEMS INCLUDING LONG-PERIOD PLANETS AND AN ECCENTRIC PLANET [PDF]

open access: green, 2015
Hiroki Harakawa   +15 more
openalex   +1 more source

Exoplanet Found in Curious Triple-Star System

open access: yesEos, 2016
The newly discovered planet balances precariously in orbit within the star system, puzzling scientists.
openaire   +2 more sources

Transiting Exoplanet Monitoring Project (TEMP). IV. Refined System Parameters, Transit Timing Variations, and Orbital Stability of the Transiting Planetary System HAT-P-25 [PDF]

open access: bronze, 2018
Xian-Yu Wang   +14 more
openalex   +1 more source

Possible Evidence for the Presence of Volatiles on the Warm Super-Earth TOI-270 b

open access: yesThe Astronomical Journal
The search for atmospheres on rocky exoplanets is a crucial step in understanding the processes driving atmosphere formation, retention, and loss. Past studies have revealed the existence of planets interior to the radius valley with densities lower than
Louis-Philippe Coulombe   +27 more
doaj   +1 more source

Transiting exoplanets from the CoRoT space mission. XXVI. CoRoT-24: a transiting multiplanet system [PDF]

open access: bronze, 2014
R. Alonso   +50 more
openalex   +1 more source

Kepler-discovered Multiple-planet Systems near Period Ratios Suggestive of Mean-motion Resonances Are Young

open access: yesThe Astronomical Journal
Before the launch of the Kepler Space Telescope, models of low-mass planet formation predicted that convergent type I migration would often produce systems of low-mass planets in low-order mean-motion resonances.
Jacob H. Hamer, Kevin C. Schlaufman
doaj   +1 more source

The Spin–Orbit Alignment of Eight Warm Gas Giant Systems

open access: yesThe Astronomical Journal
Essential information about the formation and evolution of planetary systems can be found in their architectures—in particular, in stellar obliquity ( ψ )—as they serve as a signature of their dynamical evolution. Here we present ESPRESSO observations of
Juan I. Espinoza-Retamal   +11 more
doaj   +1 more source

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