Features of the X-ray spectra of active galactic nuclei Mrk 1498

We present results of our analysis of the XMM-Newton and Swift observations of the galaxy with Sy 1.9 active nucleus Mrk 1498. We analyze the spectra obtained from three EPIC cameras (PN and both MOS) within the 0.2–12 keV energy range and Swift/BAT instrument within the range of 14-195 keV. We demo...

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Main Authors: A. A. Vasylenko, E. V. Fedorova, V. I. Zhdanov
Format: Article
Language:English
Published: National Aviation University 2013-10-01
Series:Вісник Астрономічної школи
Subjects:
Online Access:http://astro.nau.edu.ua/issues/2013_V.9_Iss.1/VasylenkoFedorovaZhdanov.html
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author A. A. Vasylenko
E. V. Fedorova
V. I. Zhdanov
author_facet A. A. Vasylenko
E. V. Fedorova
V. I. Zhdanov
author_sort A. A. Vasylenko
collection DOAJ
description We present results of our analysis of the XMM-Newton and Swift observations of the galaxy with Sy 1.9 active nucleus Mrk 1498. We analyze the spectra obtained from three EPIC cameras (PN and both MOS) within the 0.2–12 keV energy range and Swift/BAT instrument within the range of 14-195 keV. We demonstrate that for the X-ray spectrum of the AGN in this galaxy the standard models taking into account only the emission reflected by the accretion disk are adequate, but also the more complicate model including both the absorption and reflection of the primary AGN emission on a gas-dust ring shaped torus-like structure. Also, in the X-ray spectrum we detected the components corresponding to the emission of diffuse collizionally-ionized gas, and the power-law spectrum of the scattered radiation.
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spelling doaj.art-6617554079aa4a77ae1dae156666867e2022-12-22T01:52:53ZengNational Aviation UniversityВісник Астрономічної школи1607-28552411-66022013-10-0191808410.18372/2411-6602.09.10802411-6602.09.1080Features of the X-ray spectra of active galactic nuclei Mrk 1498A. A. Vasylenko0E. V. Fedorova1V. I. Zhdanov2Kyiv Shevchenko National University, UkraineKyiv Shevchenko National University, UkraineKyiv Shevchenko National University, UkraineWe present results of our analysis of the XMM-Newton and Swift observations of the galaxy with Sy 1.9 active nucleus Mrk 1498. We analyze the spectra obtained from three EPIC cameras (PN and both MOS) within the 0.2–12 keV energy range and Swift/BAT instrument within the range of 14-195 keV. We demonstrate that for the X-ray spectrum of the AGN in this galaxy the standard models taking into account only the emission reflected by the accretion disk are adequate, but also the more complicate model including both the absorption and reflection of the primary AGN emission on a gas-dust ring shaped torus-like structure. Also, in the X-ray spectrum we detected the components corresponding to the emission of diffuse collizionally-ionized gas, and the power-law spectrum of the scattered radiation.http://astro.nau.edu.ua/issues/2013_V.9_Iss.1/VasylenkoFedorovaZhdanov.htmlactive galactic nucleiX-ray spectra
spellingShingle A. A. Vasylenko
E. V. Fedorova
V. I. Zhdanov
Features of the X-ray spectra of active galactic nuclei Mrk 1498
Вісник Астрономічної школи
active galactic nuclei
X-ray spectra
title Features of the X-ray spectra of active galactic nuclei Mrk 1498
title_full Features of the X-ray spectra of active galactic nuclei Mrk 1498
title_fullStr Features of the X-ray spectra of active galactic nuclei Mrk 1498
title_full_unstemmed Features of the X-ray spectra of active galactic nuclei Mrk 1498
title_short Features of the X-ray spectra of active galactic nuclei Mrk 1498
title_sort features of the x ray spectra of active galactic nuclei mrk 1498
topic active galactic nuclei
X-ray spectra
url http://astro.nau.edu.ua/issues/2013_V.9_Iss.1/VasylenkoFedorovaZhdanov.html
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