Chemical evolution of inner regions of protoplanetary disks around T Tauri stars
This thesis has investigated the chemical evolution of the inner regions (r ≤ 10 AU) of a modelled protoplanetary disk surrounding a low-mass T Tauri star; a phase our own solar system underwent some 4.5–4.6 billion years ago. A 1+1- dimensional physical model of a radially-accreting protoplanetary...
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University of Manchester
2014
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.618034 |