X-ray polarimetric signatures induced by spectral variability in the framework of the receding torus model - INSPIRE

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X-ray polarimetric signatures induced by spectral variability in the framework of the receding torus model

F. Marin
(
- Strasbourg Observ.
)
,
R.W. Goosmann
(
- Strasbourg Observ.
)
,
P. -O. Petrucci
(
- IPAG
)

Apr 26, 2016

10 pages

Published in:

Astron.Astrophys. 591 (2016) A23

Published: Jun 6, 2016

e-Print:

1604.07562 [astro-ph.HE]

DOI:

10.1051/0004-6361/201628458

View in:

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Abstract: (EDP Sciences)

Context. Obscuring circumnuclear dust is a well-established constituent of active galactic nuclei (AGN). Traditionally referred to as the receding dusty torus, its inner radius and angular extension should depend on the photo-ionizing luminosity of the central source.

Note:

10 pages, 8 Figures, accepted for publication in A&A

galaxies: active
galaxies: Seyfert
galaxies: individual: NGC 4151
polarization
radiative transfer
X-rays: galaxies

References(83)

Figures(8)

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