X-Ray Polarimetric Observations of the Western Hotspot of Pictor A

Abstract We present the results of the analysis of a ∼2 Msec spectropolarimetric observation of the western hotspot (WHS) of the radio galaxy Pictor A. This is the brightest extragalactic radio source that allows us to carry out spatially resolved observations using the Imaging X-ray Polarimetry Explorer (IXPE) because its WHS is located at ∼250″ from the radio core. The Pictor A WHS can be detected with IXPE as a pointlike source, with very low contamination from the nuclear emission, and it is extremely polarized at both radio and optical frequencies, where its emission is well described as synchrotron radiation. We find no X-ray polarization for the Pictor A WHS. However, the derived upper limit allows us to set a first constraint on the radiative processes occurring therein, ruling out a simple synchrotron scenario where particles, with a random distribution of pitch angles, radiate in a uniform magnetic field. We also tested a scenario with a random magnetic field compressed along the jet direction.

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Publication Details

Journal
The Astrophysical Journal Letters
Published
2025-05-22
DOI
https://doi.org/10.3847/2041-8213/adcdfe
Citations
1
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
1.15

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article

X-Ray Polarimetric Observations of the Western Hotspot of Pictor A

F. Massaro, R. Bonino, Eileen T. Meyer, Herman L. Marshall et al.
1 citations
The Astrophysical Journal Letters
Astrophysical Phenomena and Observations
1.15
article

X-Ray Polarimetric Observations of the Western Hotspot of Pictor A

F. Massaro, R. Bonino, Eileen T. Meyer, Herman L. Marshall, Ioannis Liodakis, Nicolò Cibrario, S. Maldera, Eric S. Perlman, Stefano Tugliani, Michela Negro, A. Paggi, L. Latronico, A. Tramacere
article en
1 citations

Abstract

Abstract We present the results of the analysis of a ∼2 Msec spectropolarimetric observation of the western hotspot (WHS) of the radio galaxy Pictor A. This is the brightest extragalactic radio source that allows us to carry out spatially resolved observations using the Imaging X-ray Polarimetry Explorer (IXPE) because its WHS is located at ∼250″ from the radio core. The Pictor A WHS can be detected with IXPE as a pointlike source, with very low contamination from the nuclear emission, and it is extremely polarized at both radio and optical frequencies, where its emission is well described as synchrotron radiation. We find no X-ray polarization for the Pictor A WHS. However, the derived upper limit allows us to set a first constraint on the radiative processes occurring therein, ruling out a simple synchrotron scenario where particles, with a random distribution of pitch angles, radiate in a uniform magnetic field. We also tested a scenario with a random magnetic field compressed along the jet direction.

The Astrophysical Journal LettersVol. 985(2)
Florida Institute of Technology (US), University of Geneva (CH), Louisiana State University (US), Marshall Space Flight Center (US), Forthnet (Greece) (GR), Istituto Nazionale di Fisica Nucleare, Sezione di Torino (IT), Osservatorio Astrofisico di Torino (IT), University of Turin (IT), Massachusetts Institute of Technology (US), University of Maryland, Baltimore County (US)
National Aeronautics and Space Administration, European Commission
Openalex Percentile: Top 19%
Astrophysical Phenomena and Observations
1.15
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