Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/293
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dc.contributor.authorUrošević, Dejanen_US
dc.date.accessioned2022-08-06T17:48:13Z-
dc.date.available2022-08-06T17:48:13Z-
dc.date.issued2003-01-01-
dc.identifier.issn0004640Xen
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/293-
dc.description.abstractThis paper represents the updated empirical Galactic and extragalactic Σ - D relations (relations between the surface brightness Σ and the diameter D) for supernova remnants (SNRs), with checking the connection of the main Galactic radio loops (Loop I, II, III and IV) with these relations. We present results which suggest, once again, that the radio loops may have an SNR origin. The updated relations for old SNRs have been measured to have slopes, β ≈ 2 in log-log space. The best Σ - D relations for M31 and M33 galaxies were derived and these relations are shown to be flatter (β ≲ 2) than those for Galactic SNRs alone. A Σ - D relation with 168 reliable calibrators (both Galactic and extragalactic) is derived.en
dc.relation.ispartofAstrophysics and Space Scienceen
dc.subjectGalactic radio loopsen
dc.subjectSupernova remnantsen
dc.subjectΣ-D relationen
dc.titleΣ-D relations and main Galactic radio loopsen_US
dc.typeArticleen_US
dc.identifier.doi10.1023/A:1021224903880-
dc.identifier.scopus2-s2.0-0347759808-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/0347759808-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage75en
dc.relation.lastpage86en
dc.relation.volume283en
dc.relation.issue1en
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0003-0665-0939-
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