Anatomy of the AGN in NGC 5548. VIII. XMM-Newton's EPIC detailed view of an unexpected variable multilayer absorber - Archive ouverte HAL Access content directly
Journal Articles Astronomy and Astrophysics - A&A Year : 2016

Anatomy of the AGN in NGC 5548. VIII. XMM-Newton's EPIC detailed view of an unexpected variable multilayer absorber

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M. Cappi
  • Function : Author
B. de Marco
  • Function : Author
G. Ponti
  • Function : Author
S. Bianchi
J. S. Kaastra
  • Function : Author
G. A. Kriss
  • Function : Author
M. Mehdipour
M. Whewell
  • Function : Author
N. Arav
  • Function : Author
E. Behar
  • Function : Author
R. Boissay
  • Function : Author
G. Branduardi-Raymont
  • Function : Author
E. Costantini
  • Function : Author
J. Ebrero
  • Function : Author
L. Di Gesu
  • Function : Author
F. A. Harrison
  • Function : Author
S. Kaspi
  • Function : Author
G. Matt
  • Function : Author
S. Paltani
B. M. Peterson
  • Function : Author
K. C. Steenbrugge
  • Function : Author
D. J. Walton
  • Function : Author

Abstract

In 2013, we conducted a large multi-wavelength campaign on the archetypical Seyfert 1 galaxy NGC 5548. Unexpectedly, this usually unobscured source appeared strongly absorbed in the soft X-rays during the entire campaign, and signatures of new and strong outflows were present in the almost simultaneous UV HST/COS data. Here we carry out a comprehensive spectral analysis of all available XMM-Newton observations of NGC 5548 (precisely 14 observations from our campaign plus three from the archive, for a total of ~763 ks) in combination with three simultaneous NuSTAR observations. We obtain a best-fit underlying continuum model composed by I) a weakly varying flat (Γ ~ 1.5-1.7) power-law component; II) a constant, cold reflection (FeK + continuum) component; III) a soft excess, possibly owing to thermal Comptonization; and iv) a constant, ionized scattered emission-line dominated component. Our main findings are that, during the 2013 campaign, the first three of these components appear to be partially covered by a heavy and variable obscurer that is located along the line of sight (LOS), which is consistent with a multilayer of cold and mildly ionized gas. We characterize in detail the short timescale (mostly ~ks-to-days) spectral variability of this new obscurer, and find it is mostly due to a combination of column density and covering factor variations, on top of intrinsic power-law (flux and slope) variations. In addition, our best-fit spectrum is left with several (but marginal) absorption features at rest-frame energies ~6.7-6.9 keV and ~8 keV, aswell as a weak broad emission line feature redwards of the 6.4 keV emission line. These could indicate a more complex underlying model, e.g. a P-Cygni-type emission profile if we allow for a large velocity and wide-angle outflow. These findings are consistent with a picture where the obscurer represents the manifestation along the LOS of a multilayer of gas, which is also in multiphase, and which is likely outflowing at high speed, and simultaneously producing heavy obscuration and scattering in the X-rays, as well as broad absorption features in the UV.
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Dates and versions

insu-03691534 , version 1 (09-06-2022)

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M. Cappi, B. de Marco, G. Ponti, F. Ursini, P. -O. Petrucci, et al.. Anatomy of the AGN in NGC 5548. VIII. XMM-Newton's EPIC detailed view of an unexpected variable multilayer absorber. Astronomy and Astrophysics - A&A, 2016, 592, ⟨10.1051/0004-6361/201628464⟩. ⟨insu-03691534⟩
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