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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz2601
Abstract: The observed distribution of radii for exoplanets shows a bimodal form that can be explained by mass-loss from planetary atmospheres due to high-energy radiation emitted by their host stars. The location of the minimum of…
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Keywords:
magnetic fields;
effects magnetic;
mass loss;
mass ... See more keywords