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Paper detail

The soft X-ray polarization in obscured AGN

The soft X-ray emission in obscured active galactic nuclei (AGN) is dominated by emission lines, produced in a gas photoionized by the nuclear continuum and likely spatially coincident with the optical narrow line region (NLR). However, a fraction of the observed soft X-ray flux appears like a featureless power law continuum. If the continuum underlying the soft X-ray emission lines is due to Thomson scattering of the nuclear radiation, it should be very highly polarized. We calculated the expected amount of polarization assuming a simple conical geometry for the NLR, combining these results with the observed fraction of the reflected continuum in bright obscured AGN.

preprint2009arXivOpen access
Stefano BianchiGiorgio MattFrancesco TamborraMarco ChiabergeMatteo GuainazziAndrea Marinucci
astro-ph.GAastro-ph.HE
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Stefano BianchiGiorgio MattFrancesco TamborraMarco ChiabergeMatteo GuainazziAndrea Marinucci

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