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2014MNRAS.437.2806M - Mon. Not. R. Astron. Soc., 437, 2806-2815 (2014/January-3)

The variable ionized absorber in the Seyfert 2 Mrk 348.

MARCHESE E., BRAITO V., REEVES J.N., DELLA CECA R., CACCIANIGA A., MARKOWITZ A., RISALITI G., SEVERGNINI P. and TURNER T.J.

Abstract (from CDS):

We present the results of the analysis of the X-ray spectrum of the Seyfert 2 Mrk 348, observed by Suzaku and XMM-Newton. The overall spectrum of Mrk 348 can be described by a primary power-law continuum seen through three layers of absorption, of which one is neutral and two are ionized. Comparing Suzaku (2008) and XMM-Newton (2002) observations we find variability of the X-ray spectral curvature. We suggest that the variability can be explained through the change of column density of both the neutral and one of the ionized absorbers, together with a variation of the ionization level of the same absorber. We thus confirm one of the main features presented in past works, where intrinsic column density variability up to ∼ 1023/cm2 was observed on time-scales of months. We also find that the photon index of the underlying power-law continuum (Γ ∼ 1.8) is in agreement with the previous observations of this Seyfert 2.

Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)

Journal keyword(s): galaxies: active - galaxies: individual: Mrk 348 - X-rays: galaxies

Simbad objects: 10

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