Properties of soft X-ray bright Active Galactic Nuclei
Studies of the extremes of behaviour observed in Active Galactic Nuclei (AGN) constrain the physics of their emission processes by pushing existing models to their limits. Narrow-Line Seyfert 1 (NLS1s) represent one extreme of the AGN phenomenon, and soft X-ray selection is an efficient way to find...
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University of Leicester
2001
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.697003 |