X-Ray Structures in and around Powerful Radio Sources

Mathematics – Logic

Scientific paper

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Chandra Proposal Id #02700363

Scientific paper

We propose to continue our AO1 program of ACIS imaging and spectroscopy of powerful radio sources at z > 0.4. We will use temperature and density measurements of their X-ray cluster gas to study the cosmological evolution of active-galaxy environments, and how those environments affect the radio structures. We will probe the geometry and X-ray emission mechanisms of the central regions, and test that they contain unabsorbed radio-related X-ray components (as predicted by our model) even in cases where a torus of gas and dust is understood to obscure the AGN.

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