The comparative effect of FUV, EUV and X-ray disc photoevaporation on gas giant separations
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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… read more here.
Keywords: fuv euv; photoevaporation; gas; euv ray ... See more keywords