{ "id": "astro-ph/0503634", "version": "v1", "published": "2005-03-29T22:20:16.000Z", "updated": "2005-03-29T22:20:16.000Z", "title": "Discovery of Optical Emission in the Hotspots of Three 3CR Quasars: High-Energy Particle Acceleration in Powerful Radio Hotspots", "authors": [ "C. C. Cheung", "J. F. C. Wardle", "T. Chen" ], "comment": "ApJ accepted, 13 pages, downgraded quality figures for astro-ph", "journal": "Astrophys.J. 628 (2005) 104-112", "doi": "10.1086/430634", "categories": [ "astro-ph" ], "abstract": "Archival Hubble Space Telescope WFPC2 images were used to search for optical emission associated with the radio jets of a number of luminous quasars. From this search, we report new optical hotspot detections in the well-known blazar 3C~454.3 and the lobe-dominated quasars 3C~275.1 and 3C~336. We also find optical emission in the vicinity of the hotspot in 3C~208, but believe this is a chance alignment. Optical emission from the arcsecond-scale jet in 3C~454.3 is also detected. Multi-frequency archival radio data from the VLA and MERLIN are analyzed, and the synchrotron spectra of these high-power hotspots are presented. We estimate that their break frequencies are in the range of $10^{10}-10^{11}$ Hz, with large uncertainties due to the wide gap in frequency coverage between the radio and optical bands. We also calculate their equipartition magnetic fields, and find that the anti-correlation between break frequency and magnetic field found by Brunetti et al. for lower power hotspots extends to these high power hotspots. This supports their model of hot-spots based on shock acceleration and synchrotron losses.", "revisions": [ { "version": "v1", "updated": "2005-03-29T22:20:16.000Z" } ], "analyses": { "keywords": [ "optical emission", "high-energy particle acceleration", "powerful radio hotspots", "space telescope wfpc2 images", "3cr quasars" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable", "inspire": 679300 } } }