Radio properties of a complete sample of nearby groups of galaxies
Much of the evolution of galaxies takes place in groups where feedback has the greatest impact on galaxy formation. By using an optically selected, statistically complete sample of 53 nearby groups (CLoGS), observed at radio (GMRT) and X-ray (Chandra and XMM-Newton) frequencies, we aim to characteri...
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University of Birmingham
2015
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| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.655809 |