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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Видавець:Головна астрономічна обсерваторія НАН України
Дата:2015
Автори: Sadova, V.A., Tugay, A.V.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2015
Назва видання:Advances in Astronomy and Space Physics
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/119936
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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
id irk-123456789-119936
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spelling irk-123456789-1199362017-06-11T03:03:50Z The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies Sadova, V.A. Tugay, A.V. 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. 2015 Article 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 http://dspace.nbuv.gov.ua/handle/123456789/119936 en Advances in Astronomy and Space Physics Головна астрономічна обсерваторія НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
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.
format Article
author Sadova, V.A.
Tugay, A.V.
spellingShingle Sadova, V.A.
Tugay, A.V.
The luminosity - spectral index dependence of the X-ray bright Seyfert galaxies
Advances in Astronomy and Space Physics
author_facet Sadova, V.A.
Tugay, A.V.
author_sort Sadova, V.A.
title 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_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_sort luminosity - spectral index dependence of the x-ray bright seyfert galaxies
publisher Головна астрономічна обсерваторія НАН України
publishDate 2015
url http://dspace.nbuv.gov.ua/handle/123456789/119936
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.
series Advances in Astronomy and Space Physics
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