Spectral analysis of galaxies in the ultraviolet
Galaxy SEDs contain a wealth of information about their stellar populations with the UV region tracing their hot component. In young populations this hot component comes from luminous O and B-type stars whereas, in old populations a hot component can be produced after sufficient mass loss, a phenome...
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University of Portsmouth
2017
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| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.722659 |