1. Research with MATF
  2. MATF
  3. Research outputs
Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/821
DC FieldValueLanguage
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_US
dc.language.isoenen_US
dc.publisherSofia : Institute of Astronomy, Bulgarian Academy of Sciencesen_US
dc.relation.ispartofBulgarian Astronomical Journalen_US
dc.subjectISMen_US
dc.subjectISMen_US
dc.subjectMethodsen_US
dc.subjectStatisticalen_US
dc.subjectSupernova remnantsen_US
dc.subjectX-raysen_US
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.identifier.urlhttps://astro.bas.bg/AIJ/issues/n21/BArbutina.pdf-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1313-2709en_US
dc.relation.firstpage9en_US
dc.relation.lastpage14en_US
dc.relation.volume21en_US
item.openairetypeArticle-
item.fulltextNo Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-8036-4132-
Appears in Collections:Research outputs
Show simple item record

Page view(s)

25
checked on Jan 19, 2025

Google ScholarTM

Check


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.