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We present that the model of inverse Compton scattering of cosmic microwavebackground photons (IC/CMB) could well explain the large-scale jet X-rayradiation of 3C 273, and does not violate new Fermi observations. For theindividual knots, the synchrotron spectrum of the low-energy electronsresponsible for the IC/CMB X-ray emission may be different from theextrapolation of the 10GHz radio spectrum of knots. Based on the IC/CMB modelfor the 3C 273 large-scale jet, the Fermi observations may mainly come from thesmall-scale jet of 3C 273 (i.e., the core). Future observations could examineour interpretation on the spectral energy distributions (SED) of knots andlarge-scale jet in 3C 273.

An IC/CMB interpretation for the large-scale jet X-ray emission of 3C 273