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- W2079490162 abstract "We present new {it Chandra} observations of the radio galaxy 3C 445, centered on its southern radio hotspot. Our observations detect X-ray emission displaced upstream and to the west of the radio-optical hotspot. Attempting to reproduce both the observed spectral energy distribution (SED) and the displacement, excludes all one zone models. Modeling of the radio-optical hotspot spectrum suggests that the electron distribution has a low energy cutoff or break approximately at the proton rest mass energy. The X-rays could be due to external Compton scattering of the cosmic microwave background (EC/CMB) coming from the fast (Lorentz factor $Gammaapprox 4$) part of a decelerating flow, but this requires a small angle between the jet velocity and the observer's line of sight ($thetaapprox 14^{circ}$). Alternatively, the X-ray emission can be synchrotron from a separate population of electrons. This last interpretation does not require the X-ray emission to be beamed." @default.
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- W2079490162 date "2009-12-08" @default.
- W2079490162 modified "2023-10-09" @default.
- W2079490162 title "<i>CHANDRA</i>OBSERVATIONS OF THE RADIO GALAXY 3C 445 AND THE HOT SPOT X-RAY EMISSION MECHANISM" @default.
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- W2079490162 doi "https://doi.org/10.1088/0004-637x/708/1/1" @default.
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