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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/821
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dc.contributor.authorArbutina, Bojanen_US
dc.date.accessioned2022-08-15T16:03:22Z-
dc.date.available2022-08-15T16:03:22Z-
dc.date.issued2014-01-01-
dc.identifier.issn13132709en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/821-
dc.description.abstractThis paper introduces a sort of“H-R diagram” i.e. L<inf>X</inf>-kT diagram for supernova remnants (SNRs). Although the example given in this paper is only illustrative and the models discussed too simplistic, further investigation of this topic may hold some promise for better understanding of the evolution of SNRs.en
dc.relation.ispartofBulgarian Astronomical Journalen
dc.subjectISMen
dc.subjectISMen
dc.subjectMethodsen
dc.subjectStatisticalen
dc.subjectSupernova remnantsen
dc.subjectX-raysen
dc.titleThe H-R diagram for supernova remnantsen_US
dc.typeArticleen_US
dc.identifier.scopus2-s2.0-84929393964-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84929393964-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage9en
dc.relation.lastpage14en
dc.relation.volume21en
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-8036-4132-
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