The influence of a migrating planet on the topology and chemistry of a protoplanetary disc
One of the surprising discoveries in the field of extrasolar planets is the proliferation of massive planets in small orbits. It is not believed possible for these planets to form in situ. Instead, it is likely that they formed at much greater distances from their parent stars, beyond the radial dis...
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University College London (University of London)
2009
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.625200 |