Computer Science
Scientific paper
Oct 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...79p&link_type=abstract
XMM-Newton Proposal ID #03023103
Computer Science
Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Rxj163309+57025, Rxj163309+57025, Rxj005734-27282, Xmm-Newton Proposal 03023103
Scientific paper
According to galaxy formation models, cluster ellipticals formed in high density regions through hierarchical merging of gas rich sub-components. In local ellipticals, the strong correlation observed between black hole and bulge mass implies that galaxy formation is inextricably linked to the build up of supermassive black holes. We have found 6 high redshift, X-ray luminous, but heavily absorbed AGN, embedded in strong bursts of star formation revealed in the submillimetre. Our SCUBA survey shows that the immediate vicinities of these objects contain large over-densities of ultraluminous star-forming galaxies which will evolve to form clusters. Here we propose to use XMM-Newton to observe the early evolutionary phases of QSOs in these proto-clusters.
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