Very high energy gamma ray astronomy and non pulsating low mass X-ray binaries
This thesis is concerned with non pulsating Low Mass X-Ray Binaries as Very High Energy γ-ray sources, in particular Scorpius X-1; the brightest of these objects in X-rays, and the most likely to be detectable at energies above 250 GeV. After a first introductory chapter, experimental techniques pre...
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Durham University
1991
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.317308 |