Dust in the centres of galaxies : observations and modelling of dust in the nucleus of NGC1068 and in the galactic centre
The 'archetypal' Seyfert II galaxy, NGC1068, is one of the best-studied dusty objects in the sky. Yet - in common with Seyfert galaxies in general - the properties of its dust are not at all well-known. To remedy this situation I have modelled the IR polarisation and 3.4/rm dust absorption...
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University of Edinburgh
2003
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.735412 |