{ "id": "astro-ph/0106029", "version": "v2", "published": "2001-06-01T22:14:48.000Z", "updated": "2001-06-07T13:28:25.000Z", "title": "Chandra observations of the X-ray jet in 3C66B", "authors": [ "M. J. Hardcastle", "M. Birkinshaw", "D. M. Worrall" ], "comment": "9 pages, 6 figures. MNRAS accepted. v2; fix typo in core spectral index and UGC number", "journal": "Mon.Not.Roy.Astron.Soc. 326 (2001) 1499", "categories": [ "astro-ph" ], "abstract": "Our Chandra observation of the FRI radio galaxy 3C66B has resulted in the first detection of an X-ray counterpart to the previously known radio, infra-red and optical jet. The X-ray jet is detected up to 7 arcsec from the core and has a steep X-ray spectrum, alpha ~ 1.3 +/- 0.1. The overall X-ray flux density and spectrum of the jet are consistent with a synchrotron origin for the X-ray emission. However, the inner knot in the jet has a higher ratio of X-ray to radio emission than the others. This suggests that either two distinct emission processes are present or that differences in the acceleration mechanism are required; there may be a contribution to the inner knot's emission from an inverse-Compton process or it may be the site of an early strong shock in the jet. The peak of the brightest radio and X-ray knot is significantly closer to the nucleus in the X-ray than in the radio, which may suggest that the knots are privileged sites for high-energy particle acceleration. 3C66B's jet is similar both in overall spectral shape and in structural detail to those in more nearby sources such as M87 and Centaurus A.", "revisions": [ { "version": "v2", "updated": "2001-06-07T13:28:25.000Z" } ], "analyses": { "keywords": [ "chandra observation", "x-ray jet", "fri radio galaxy 3c66b", "overall x-ray flux density", "overall spectral shape" ], "tags": [ "journal article" ], "publication": { "doi": "10.1111/j.1365-2966.2001.04699.x" }, "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable", "inspire": 575201 } } }