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

dc.contributor.authorSadova, V.A.
dc.contributor.authorTugay, A.V.
dc.date.accessioned2017-06-10T12:06:00Z
dc.date.available2017-06-10T12:06:00Z
dc.date.issued2015
dc.description.abstractX-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.uk_UA
dc.description.sponsorshipThis 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.uk_UA
dc.identifier.citationThe 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.uk_UA
dc.identifier.issn2227-1481
dc.identifier.otherDOI:10.17721/2227-1481.5.79-83
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/119936
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleThe luminosity - spectral index dependence of the X-ray bright Seyfert galaxiesuk_UA
dc.typeArticleuk_UA

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