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P. Kaaret (Harvard-Smithsonian CfA)
Properties of the x-ray sources detected with Chandra in M82 are described, concentrating on the most luminous source. The x-ray images are compared with infrared and radio images to attempt to identify counterparts for the x-ray sources.
The author(s) of this abstract have provided an email address for comments about the abstract: pkaaret@cfa.harvard.edu