A time-resolved study of the injection of mass onto a dormant Supermassive Black

Details A time-resolved study of the injection of mass onto a dormant Supermassive Black A time-resolved study of the injection of mass onto a dormant Supermassive Black

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop..157s&link_type=abstract

XMM-Newton Proposal ID #05550601

Computer Science

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Galaxy 1, Xmm-Newton Proposal Id #05550601

Scientific paper

The near real-time comparison of XMM-Newton slew data with the ROSAT all-sky survey gives an excellent opportunity to find black holes in the centres of galaxies, which are currently being fueled by the tidal disruption of a star. The intensive study of such a system, where the boundary conditions, i.e. the recent history of the nuclear radiation, are known, will provide sensitive diagnostics in several areas of the AGN phenomenon,which are at best ambiguous when viewed in a 'steady-state' AGN. We propose to follow the dynamical evolution of the accretion process by studying the X-ray, UV and optical emission with regular observations to measure the evolution of the spectral components.

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