arXiv · 0909.3645
Suzaku Observations of the Radio Galaxy 3C 33
Abstract
We present results from a new 100-ks Suzaku observation of the nearby radio galaxy 3C 33, and investigate the nature of absorption, reflection, and jet production in this source. We model the 2-70 keV nuclear continuum with a power law that is absorbed either through one or more layers of pc-scale neutral material, or through a modestly ionized pc-scale obscurer. The expected signatures of reflection from a neutral accretion disk are absent in 3C 33: there is no evidence of a relativistically blurred Fe K$α$ emission line, and no Compton reflection hump above 10 keV. We discuss the implications of this for the nature of jet production in 3C 33.
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Daniel A. Evans, James N. Reeves, Martin J. Hardcastle, Ralph P. Kraft, Julia C. Lee, Shanil N. Virani. 2009-09-20. Suzaku Observations of the Radio Galaxy 3C 33. https://arxiv.org/abs/0909.3645
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