Production of diamond using intense heavy ion beams at the FAIR facility and application to planetary physics. [PDF]
Sci Rep, 2023 Tahir NA +4 more
europepmc +1 more source
Semianalytical Accretion-tracer Emission: Forming Planets Are Intrinsically Faint
The Astrophysical JournalDirect-imaging surveys have looked for accreting planets through their accretion tracers such as H α but have been less fruitful than expected.
Gabriel-Dominique Marleau
doaj +1 more source
A comprehensive investigation of the Galilean moon, Io, by tracing mass and energy flows. [PDF]
Exp Astron (Dordr), 2022 Thomas N.
europepmc +1 more source
The Roman Microlensing Survey: Confirmation or Refutation of Gas Giant Exoplanet Formation Theories
The Astrophysical JournalExoplanet 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
doaj +1 more source
Infrared Spectra of Small Radicals for Exoplanetary Spectroscopy: OH, NH, CN and CH: The State of Current Knowledge. [PDF]
Molecules, 2023 Civiš S +4 more
europepmc +1 more source
, 2021 Beyond the Solar System there are more than 3000 stellar systems composed of since dwarfs to supergiant stars, orbited by more than 4000 exoplanets divided in several types, small and rocky, giant and gaseous, some of which are not seen in the Solar ...
Bezerra, Brandon Oliveira
core
The Heating Efficiency of Hot Jupiters from a Data-driven Perspective
The Astronomical JournalThe inflated radii of hot Jupiters have been explored by various theoretical mechanisms. By connecting planetary thermal evolution models with the observed properties of hot Jupiters using hierarchical Bayesian models, a theoretical parameter called the ...
Sheng Jin +3 more
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, 2021 Ilustraciones y tablasRecent advances in exoplanet observations have led to the discovery of nearly 4400 planets in more than 3000 planetary systems. However, many physical properties of these systems remain largely unknown due to observational biases ...
Bautista Sánchez, Frank Jair
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Relative Occurrence Rate between Hot and Cold Jupiters as an Indicator to Probe Planet Migration
The Astrophysical JournalWe propose a second-order statistic parameter ε , the relative occurrence rate between hot Jupiters (HJs) and cold Jupiters (CJs) ( ε = η _HJ / η _CJ ), to probe the migration of gas giants. Since the planet occurrence rate is the combined outcome of the
Tianjun Gan +6 more
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Identification of carbon dioxide in an exoplanet atmosphere. [PDF]
Nature, 2023 JWST Transiting Exoplanet Community Early Release Science Team.
europepmc +1 more source