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We present results from Suzaku and Swift observations of the nearby radiogalaxy 3C 33, and investigate the nature of absorption, reflection, and jetproduction in this source. We model the 0.5-100 keV nuclear continuum with apower law that is transmitted either through one or more layers of pc-scaleneutral material, or through a modestly ionized pc-scale obscurer. The standardsignatures of reflection from a neutral accretion disk are absent in 3C 33:there is no evidence of a relativistically blurred Fe K$\alpha$ emission line,and no Compton reflection hump above 10 keV. We find the upper limit to theneutral reflection fraction is R<0.41 for an e-folding energy of 1 GeV. Weobserve a narrow, neutral Fe K$\alpha$ line, which is likely to originate atleast 2,000 R_s from the black hole. We show that the weakness of reflectionfeatures in 3C 33 is consistent with two interpretations: either the inneraccretion flow is highly ionized, or the black-hole spin configuration isretrograde with respect to the accreting material.

The Hard X-Ray View of Reflection, Absorption, and the Disk-Jet Connection in the Radio-Loud AGN 3C 33