Predicting the X-ray polarization of type-2 Seyfert galaxies

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Marin , F.; Dovciak , M.; Muleri , F.; Kislat , F.F.; Krawczynski , H.S.;
  • Publisher: HAL CCSD
  • Related identifiers: doi: 10.1093/mnras/stx2382
  • Subject: relativistic processes | X-rays: general | scattering | galaxies: active | radiative transfer | [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] | polarization | [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]
    arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::High Energy Astrophysical Phenomena | Astrophysics::Cosmology and Extragalactic Astrophysics

International audience; Infrared, optical and ultraviolet spectropolarimetric observations have proven to be ideal tools for the study of the hidden nuclei of type 2 active galactic nuclei (AGN) and for constraining the composition and morphology of the sub-parsec scale... View more
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