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arXiv · astro-ph/0602021

An optical-IR jet in 3C133

David J. E. Floyd·Robert Laing·Marco Chiaberge·Eric Perlman·William Sparks·Duccio Macchetto·Juan Madrid·David Axon·Christopher P. O'Dea·Stefi Baum·Alice Quillen·George Miley·Alessandro Capetti
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Abstract

We report the discovery of a new optical-IR synchrotron jet in the radio galaxy 3C133 from our HST/NICMOS snapshot survey. The jet and eastern hotspot are well resolved, and visible at both optical and IR wavelengths. The IR jet follows the morphology of the inner part of the radio jet, with three distinct knots identified with features in the radio. The radio-IR SED's of the knots are examined, along with those of two more distant hotspots at the eastern extreme of the radio feature. The detected emission appears to be synchrotron, with peaks in the NIR for all except one case, which exhibits a power-law spectrum throughout.

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David J. E. Floyd, Robert Laing, Marco Chiaberge, Eric Perlman, William Sparks, Duccio Macchetto, Juan Madrid, David Axon, Christopher P. O'Dea, Stefi Baum, Alice Quillen, George Miley, Alessandro Capetti. 2006-02-01. An optical-IR jet in 3C133. https://doi.org/10.1086/503027

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