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Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty964
Abstract: Gas giants' early (less than or similar to 5 Myr) orbital evolution occurs in a disc losing mass in part to photoevaporation driven by high energy irradiance from the host star. This process may ultimately…
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Keywords:
fuv euv;
photoevaporation;
gas;
euv ray ... See more keywords