Detecting ring systems around exoplanets using high resolution spectroscopy: the case of 51 Pegasi b [PDF]
N. C. Santos +15 more
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FIVE NEW EXOPLANETS ORBITING THREE METAL-RICH, MASSIVE STARS: TWO-PLANET SYSTEMS INCLUDING LONG-PERIOD PLANETS AND AN ECCENTRIC PLANET [PDF]
Hiroki Harakawa +15 more
openalex +1 more source
Exoplanet Found in Curious Triple-Star System
The newly discovered planet balances precariously in orbit within the star system, puzzling scientists.
openaire +2 more sources
A Search for Lost Planets in the Kepler Multi-planet Systems and the Discovery of the Long-period, Neptune-sized Exoplanet Kepler-150 f [PDF]
Joseph R. Schmitt +2 more
openalex +1 more source
Transiting Exoplanet Monitoring Project (TEMP). IV. Refined System Parameters, Transit Timing Variations, and Orbital Stability of the Transiting Planetary System HAT-P-25 [PDF]
Xian-Yu Wang +14 more
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Possible Evidence for the Presence of Volatiles on the Warm Super-Earth TOI-270 b
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
The search for radio emission from exoplanets using LOFAR low-frequency beamformed observations: Data pipeline and preliminary results for the 55 Cnc system [PDF]
Jake D. Turner +3 more
openalex +1 more source
Transiting exoplanets from the CoRoT space mission. XXVI. CoRoT-24: a transiting multiplanet system [PDF]
R. Alonso +50 more
openalex +1 more source
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
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
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