Fig. 9
SEDs of the synchrotron and IC emission for the starburst galaxies. The top panel corresponds to 3C 273, and the bottom panel to Mrk 231. In both panels, solid lines correspond to a magnetic field in equipartition with the jet ram pressure, and dashed lines to the case below equipartition. Radio data for both sources are also presented, along with Fermi detection and HESS upper limits for 3C 273.
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