X-ray spectroscopy of active galactic nuclei
This thesis was triggered by the question what is the nature of the sources producing the bulk of the X-ray background at hard energies. Of course the pre-Chandra missions did not allow any definite answer to this question. Therefore the approach adopted in this work is to examine whether candidate...
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University of Leicester
2001
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.696993 |