Modelling of the upper atmosphere of gas-giant exoplanets irradiated by low-mass stars
Upper atmospheres of Hot Jupiters are subject to extreme radiation conditions that can result in rapid atmospheric escape. The composition and structure of the upper atmosphere of these planets are affected by the high-energy spectrum of the host star. This emission depends on stellar type and age,...
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Imperial College London
2015
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.676801 |