The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies

X-ray luminosities and spectral indices of 97 bright Seyfert 1 (Sy1) galaxies from the XMM-Newton archive are analysed in this article. Distribution of these values is random, so we conclude that the model of emission should be at least two-parametric. Within the framework of the merging model of ac...

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Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2015
Автори: Sadova, V.A., Tugay, A.V.
Формат: Стаття
Мова:Англійська
Опубліковано: Головна астрономічна обсерваторія НАН України 2015
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/119936
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies / V.A. Sadova, A.V. Tugay // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 2. — С. 79-83. — Бібліогр.: 22 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Sadova, V.A.
Tugay, A.V.
author_facet Sadova, V.A.
Tugay, A.V.
citation_txt The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies / V.A. Sadova, A.V. Tugay // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 2. — С. 79-83. — Бібліогр.: 22 назв. — англ.
collection DSpace DC
container_title Advances in Astronomy and Space Physics
description X-ray luminosities and spectral indices of 97 bright Seyfert 1 (Sy1) galaxies from the XMM-Newton archive are analysed in this article. Distribution of these values is random, so we conclude that the model of emission should be at least two-parametric. Within the framework of the merging model of active galactic nuclei (AGN), the relation between black hole mass, stage of merging and observable X-ray parameters is roposed.
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last_indexed 2025-12-07T20:54:40Z
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publisher Головна астрономічна обсерваторія НАН України
record_format dspace
spelling Sadova, V.A.
Tugay, A.V.
2017-06-10T12:06:00Z
2017-06-10T12:06:00Z
2015
The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies / V.A. Sadova, A.V. Tugay // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 2. — С. 79-83. — Бібліогр.: 22 назв. — англ.
2227-1481
DOI:10.17721/2227-1481.5.79-83
https://nasplib.isofts.kiev.ua/handle/123456789/119936
X-ray luminosities and spectral indices of 97 bright Seyfert 1 (Sy1) galaxies from the XMM-Newton archive are analysed in this article. Distribution of these values is random, so we conclude that the model of emission should be at least two-parametric. Within the framework of the merging model of active galactic nuclei (AGN), the relation between black hole mass, stage of merging and observable X-ray parameters is roposed.
This work was performed at VIRGO.UA. The authors are thankful to the ISDC High-Energy Astrophysics Data Centre for developing the Ukrainian Virtual Roentgen and Gamma Observatory. A. Tugay thanks to anonymous referee for useful comments.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies
Article
published earlier
spellingShingle The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies
Sadova, V.A.
Tugay, A.V.
title The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies
title_full The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies
title_fullStr The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies
title_full_unstemmed The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies
title_short The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies
title_sort luminosity - spectral index dependence of the x-ray bright seyfert galaxies
url https://nasplib.isofts.kiev.ua/handle/123456789/119936
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