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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/116
DC FieldValueLanguage
dc.contributor.authorIlić, Draganaen_US
dc.date.accessioned2022-08-06T15:18:35Z-
dc.date.available2022-08-06T15:18:35Z-
dc.date.issued2007-12-01-
dc.identifier.issn1450698Xen
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/116-
dc.description.abstractIn this paper an analysis of the physical properties of the Broad Line Region (BLR) of the active galaxy NGC 5548 is presented. Using the photoionization code CLOUDY and the measurements of Peterson et al. (2002), the physical conditions of the BLR are simulated and the BLR temperature is obtained. This temperature was compared to the temperature estimated with the Boltzmann-Plot (BP) method (Popović et al. 2007). It was shown that the measured variability in the BLR temperature could be due to the change in the hydrogen density.en_US
dc.language.isoenen_US
dc.publisherBeograd : Matematički fakulteten_US
dc.relation.ispartofSerbian Astronomical Journalen_US
dc.subjectGalaxies: activeen_US
dc.subjectGalaxies: individual: NGC 5548en_US
dc.subjectGalaxies: Seyferten_US
dc.subjectLine: formationen_US
dc.subjectPlasmasen_US
dc.titleSimulations of the broad line region of NGC 5548 with cloudy code: Temperature determinationen_US
dc.typeArticleen_US
dc.identifier.doi10.2298/SAJ0775015I-
dc.identifier.scopus2-s2.0-38549120368-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/38549120368-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1450-698Xen_US
dc.relation.firstpage15en_US
dc.relation.lastpage18en_US
dc.relation.issue175en_US
item.openairetypeArticle-
item.languageiso639-1en-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-1134-4015-
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