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M. W. Bautz (MIT Center for Space Research)
I present and discuss deep Chandra images of a number of galaxy clusters, some of which are strong gravitational lenses. I describe the X-ray properties of lensed background objects in these fields, and discuss the implications of these new Chandra detections for the X-ray/sub-millimeter connection. I present spatially resolved X-ray spectroscopy of the core cluster emission, and consider its implications for the dynamical state and mass distributions of these objects.
This work was supported by NASA.
The author(s) of this abstract have provided an email address for comments about the abstract: mwb@space.mit.edu