XMM-Newton Proposal 02025205

Details XMM-Newton Proposal 02025205 XMM-Newton Proposal 02025205

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..133s&link_type=abstract

XMM-Newton Proposal ID #02025205

Physics

B0108+388, B0710+439, B1031+567, B1358+624, B2352+495, Xmm-Newton Proposal 02025205

Scientific paper

The new X-ray observatories have given us great insights into the energetic accretion processes in active galaxies, providing important clues about possible connections between different classes of radio-quiet and radio-loud AGN. Although much of the current work is focused on parameterizing the X-ray emission of AGN, virtually nothing is known about the possible evolution of the X-ray properties over the lifetime of an AGN. We propose to perform the first X-ray observations of the 5 most famous and extensively studied young GPS radio galaxies in the sky. This will yield important information on the evolution of the accretion flow over the AGN-lifecycle, and the mass and distribution of circumnuclear material around young radio sources.

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