ALMA ACA detection of submillimeter emission associated with the west hot spot of the radio galaxy Pictor A
arXiv:2306.14950 · doi:10.3847/1538-4357/ace04d
Abstract
In order to investigate the far-infrared excess detected from the west hot spot of the radio galaxy Pictor A with the Herschel observatory, a submillimeter photometry is performed with the Atacama Compact Array (ACA) of the Atacama Large Millimeter/submillimeter Array at Band 8 with the reference frequency of 405 GHz. A submillimeter source is discovered at the radio peak of the hot spot. Because the 405 GHz flux density of the source, mJy, agrees with the extrapolation of the synchrotron radio spectrum, the far-infrared excess is suggested to exhibit no major contribution at the ACA band. In contrast, by subtracting the power-law spectrum tightly constrained by the radio and ACA data, the significance of the excess in the Herschel band is well confirmed. No diffuse submillimeter emission is detected within the ACA field of view, and thus, the excess is ascribed to the west hot spot itself. In comparison to the previous estimate based on the Herschel data, the relative contribution of the far-infrared excess is reduced by a factor of . The spectrum of the excess below the far-infrared band is determined to be harder than that of the diffusive shock acceleration. This strengthens the previous interpretation that the excess originates via the magnetic turbulence in the substructures within the hot spot. The ACA data are utilized to evaluate the magnetic field strength of the excess and of diffuse radio structure associated to the hot spot.
arXiv comment10 pages,4 figures, 3 tables, accepted for ApJ
References in corpus (25)
- Astropy: A Community Python Package for Astronomy
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- The Herschel-SPIRE instrument and its in-flight performance
- Relativistic Reconnection: an Efficient Source of Non-Thermal Particles
- An Accurate Flux Density Scale from 50 MHz to 50 GHz
- Fine Structures of Shock of SN 1006 with the Chandra Observation
- Turbulence and Magnetic Field Amplification in Supernova Remnants: Interactions Between A Strong Shock Wave and Multi-Phase Interstellar Medium
- The origins of X-ray emission from the hotspots of FRII radio sources
- Flux Calibration of Broadband Far Infrared and Submillimetre Photometric Instruments: Theory and Application to Herschel-SPIRE
- Accurate Redshifts and Classifications for 110 Radio-Loud AGNs
- Time-Dependent Models for Blazar Emissions with the Second-Order Fermi Acceleration
- Constraints on the energetics and plasma composition of relativistic jets in FR II sources
- Magnetic Field Amplification by Turbulence in A Relativistic Shock Propagating through An Inhomogeneous Medium
- A high resolution view of the jet termination shock in a hot spot of the nearby radio galaxy Pictor A: implications for X-ray models of radio galaxy hot spots
- Anisotropic inverse Compton scattering in powerful radio galaxies: the case of 3C 295
- Complex shock structure in the western hot-spot of Pictor A
- Hysteresis of Backflow Imprinted in Collimated Jets
- Calorimetry of Active Galactic Nucleus jets: testing plasma composition in Cygnus A
- Evidence for a significant mixture of electron/positron pairs in FRII jets constrained by cocoon dynamics
- Mid-infrared excess from the west hot spot of the radio galaxy Pictor A unveiled by WISE
- ALMA polarization observations of the particle accelerators in the hot spot of the radio galaxy 3C 445
- Herschel SPIRE discovery of far-infrared excess synchrotron emission from the west hot spot of the radio galaxy Pictor A
- discovery of far-infrared emission from the hot spot D in the radio galaxy Cygnus A