The physical properties and composition of Vega-type disks
The first part of the thesis presents new sub-mm observations of Vega excess stars, and modelling for all known Vega excess stars which have sub-mm data, using dust grain models with realistic optical properties. Analysis of there solved targets showed that different objects require very different d...
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University of Edinburgh
2005
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.661849 |