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 cm−2 was observed on time-scales of months. We also find that the photon index of the underlying power-law continuum ( ∼ 1.8) is in agreement with the previous observations of this Seyfert 2.

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.; Turner, T. J.. - In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. - ISSN 1365-2966. - STAMPA. - 437:(2014), pp. 2806-2815. [10.1093/mnras/stt2101]

The variable ionized absorber in the Seyfert 2 Mrk 348

RISALITI, GUIDO;
2014

Abstract

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 cm−2 was observed on time-scales of months. We also find that the photon index of the underlying power-law continuum ( ∼ 1.8) is in agreement with the previous observations of this Seyfert 2.
2014
437
2806
2815
Marchese, E.; Braito, V.; Reeves, J. N.; Della Ceca, R.; Caccianiga, A.; Markowitz, A.; Risaliti, G.; Severgnini, P.; Turner, T. J.
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1078234
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