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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2785
DC FieldValueLanguage
dc.contributor.authorArbutina, Bojanen_US
dc.contributor.authorOpsenica, Slobodanen_US
dc.date.accessioned2025-10-20T08:53:48Z-
dc.date.available2025-10-20T08:53:48Z-
dc.date.issued2012-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2785-
dc.description.abstractExpressions for surface brightness distribution and for flux density have been theoretically derived in the case of two simple models of a shell supernova remnant. The models are: a homogenous optically thin emitting shell with constant emissivity and a synchrotron shell source with radial magnetic field. Interactive Data Language (IDL) codes for fitting theoretically derived emission profiles assuming these two models to mean profiles of shell supernova remnants obtained from radio observations have been written.en_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomska opservatorijaen_US
dc.relation.ispartofPublications of the Astronomical observatory Belgradeen_US
dc.titleNumerical Code for Fitting Radial Emission Profile of a Shell Supernova Remnanten_US
dc.typeConference Objecten_US
dc.relation.conferenceNational Conference of Serbian Astronomers (16 ; 2011 ; Beograd)en_US
dc.relation.publicationProceedings of the 16th National Conference of Astronomers of Serbiaen_US
dc.identifier.urlhttps://arxiv.org/abs/1201.0855-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0373-3742en_US
dc.description.rankM63en_US
dc.relation.firstpage331en_US
dc.relation.lastpage335en_US
dc.relation.volume91en_US
item.openairetypeConference Object-
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-
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