Herschel SPIRE discovery of far-infrared excess synchrotron emission from the west hot spot of the radio galaxy Pictor A
arXiv:2006.10737 · doi:10.3847/1538-4357/ab9d1c
Abstract
A far-infrared counterpart to the west hot spot of the radio galaxy Pictor A is discovered with the Spectral and Photometric Imaging REceiver (SPIRE) onboard Herschel. The color-corrected flux density of the source is measured as mJy at the wavelength of 350 m. A close investigation into its radio-to-optical spectrum indicates that the mid-infrared excess over the radio synchrotron component, detected with WISE and Spitzer, significantly contributes to the far-infrared band. Thanks to the SPIRE data, it is revealed that the spectrum of the excess is described by a broken power-law model subjected to a high-energy cutoff. By applying the radiative cooling break under continuous energy injection (), the broken power-law model supports an idea that the excess originates in 10-pc scale substructures within the hot spot. From the break frequency, Hz, the magnetic field was estimated as - mG. This is higher than the minimum-energy magnetic field of the substructures by a factor of --. Even if the origin of the excess is larger than pc, the magnetic field stronger than the minimum-energy field is confirmed. It is proposed that regions with a magnetic field locally boosted via plasma turbulence are observed as the substructures. The derived energy index below the break, (conservatively ), is difficult to be attributed to the strong-shock acceleration (). Stochastic acceleration and magnetic reconnection are considered as a plausible alternative mechanism.
arXiv comment13 pages, 3 figures, 4 tables, accepted for ApJ
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