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

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

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop..166s&link_type=abstract

XMM-Newton Proposal ID #06739002

Computer Science

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Galaxy 3, Galaxy 3

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 systems, where the boundary conditions, i.e. the recent history of the nuclear radiation, are known, can provide sensitive diagnostics in several areas of the AGN phenomenon. We propose to follow the dynamical evolution of the accretion process by studying the X-ray, UV and optical emission with regular observations. In AO9, this program was triggered on SDSS~J120136.02+300305.5, which has worked as a proof of concept. More events will allow the evolution to be followed for systems with different SMBH masses and stellar progenitors.

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