Mapping the circumnuclear regions of the Circinus galaxy with the Imaging X-ray Polarimetry Explorer
arXiv:2211.01697 · doi:10.1093/mnras/stac3189
Abstract
We report on the Imaging X-ray Polarimetry Explorer (IXPE) observation of the closest and X-ray brightest Compton-thick active galactic nucleus (AGN), the Circinus galaxy. We find the source to be significantly polarized in the 2--6 keV band. From previous studies, the X-ray spectrum is known to be dominated by reflection components, both neutral (torus) and ionized (ionization cones). Our analysis indicates that the polarization degree is per cent (at 68 per cent confidence level) for the neutral reflector, with a polarization angle of , roughly perpendicular to the radio jet. The polarization of the ionized reflection is unconstrained. A comparison with Monte Carlo simulations of the polarization expected from the torus shows that the neutral reflector is consistent with being an equatorial torus with a half-opening angle of 45°-55°. This is the first X-ray polarization detection in a Seyfert galaxy, demonstrating the power of X-ray polarimetry in probing the geometry of the circumnuclear regions of AGNs, and confirming the basic predictions of standard Unification Models.
9 pages, accepted for publication in MNRAS, authors list updated
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- X-ray polarization from accretion disk winds
- X-ray polarization measurement of the gold standard of radio-quiet active galactic nuclei : NGC 1068
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- Spectral and polarization properties of reflected X-ray emission from black-hole accretion discs for a distant observer: the lamp-post model
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- Multi-epoch hard X-ray view of Compton-thick AGN Circinus Galaxy
- The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3
- Enhanced activity in close dual-AGN systems in the local Universe
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