Many details of the gas accretion phase during giant planet formation remain untested. We present new 0.2–0.7 μ m UV-through-red optical imaging of the young, wide-orbit planetary-mass companion SR 12 c from the Wide Field Camera 3 (WFC3) instrument on ...
Claire O. Finley +14 more
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Solving protoplanetary structure equations using Adomian decomposition method. [PDF]
Paul GC +6 more
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The Roman Microlensing Survey: Confirmation or Refutation of Gas Giant Exoplanet Formation Theories
Exoplanet research has moved from the discovery of new classes of planets toward creating a census of exoplanet population demographics across the spectrum of exoplanet and host star masses.
Alan P. Boss
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Infrared Spectra of Small Radicals for Exoplanetary Spectroscopy: OH, NH, CN and CH: The State of Current Knowledge. [PDF]
Civiš S +4 more
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Ice giant system exploration in the 2020s: an introduction. [PDF]
Fletcher LN +7 more
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Potential sublimating exocomets around the young star PDS 70. [PDF]
Novais A +6 more
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The onset of collective diffusion in hcp-iron: a combined theory of soft-matter and solid-state physics. [PDF]
Cuong TD, Phan AD.
europepmc +1 more source
Exploring exoplanet dynamics with JWST: Tides, rotation, rings, and moons. [PDF]
Millholland SC, Winn JN.
europepmc +1 more source
Planets larger than Neptune have elevated eccentricities. [PDF]
Gilbert GJ, Petigura EA, Entrican PM.
europepmc +1 more source
Formation of exoplanetary satellites by pull-down capture. [PDF]
Hansen BMS.
europepmc +1 more source

