Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? [PDF]
, 2022 C. Swastik +7 more
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Structure and evolution of super-Earth to super-Jupiter exoplanets [PDF]
, 2008 I. Baraffe, G. Chabrier, Travis Barman
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The Astronomical JournalBefore 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
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Can Isotopologues Be Used as Biosignature Gases in Exoplanet Atmospheres? [PDF]
Life (Basel), 2023 Glidden A +3 more
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LITHIUM ABUNDANCES IN NEARBY FGK DWARF AND SUBGIANT STARS: INTERNAL DESTRUCTION, GALACTIC CHEMICAL EVOLUTION, AND EXOPLANETS [PDF]
, 2012 I. Ramírez +3 more
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Temporal Evolution of the High-energy Irradiation and Water Content of TRAPPIST-1 Exoplanets [PDF]
, 2017 V. Bourrier +15 more
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Main-sequence exoplanet systems: tidal evolution
The easiest exoplanets to detect are those that orbit very close to their hoststars. As a result, even though these planets are quite rare, they represent amajor fraction of the current exoplanet population. A side-effect of theproximity between the planet and the star is that the two have strong mutualinteractions through a number of physical ...
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Thermal evolution of rocky exoplanets with a graphite outer shell [PDF]
, 2019 Kaustubh Hakim +5 more
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The influence of bulk composition on the long-term interior-atmosphere evolution of terrestrial exoplanets [PDF]
, 2020 Rob Spaargaren +4 more
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A Coupled Analysis of Atmospheric Mass Loss and Tidal Evolution in XUV Irradiated Exoplanets: The TRAPPIST-1 Case Study [PDF]
, 2020 Juliette Becker +4 more
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