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Clusters of galaxies are strong emitters of EUV and soft X-rays substantiallyin excess of the contribution from the hot intra-cluster medium at X-raytemperatures. After the initial discovery of EUV excess emission in the Virgocluster, the phenomenon was reported also for the Coma, A1795 and A2199clusters. Recent reobservations confirmed the finding, and further searches ona large sample of nearby galaxy clusters are clearly revealing the cosmologicalimpact of the discovery.Comment: An invited review at the International Dark Matter meeting IDM2000,  Sept 2000, York (England

EUV AND SOFT X–RAYS FROM CLUSTERS OF GALAXIES – THE 'CLUSTER SOFT–EXCESS' PHENOMENON