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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2928
DC FieldValueLanguage
dc.contributor.authorBorka Jovanović, Vesnaen_US
dc.contributor.authorMilogradov-Turin, Jelenaen_US
dc.contributor.authorUrošević, Dejanen_US
dc.date.accessioned2025-11-25T14:45:20Z-
dc.date.available2025-11-25T14:45:20Z-
dc.date.issued2006-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2928-
dc.description.abstractIn this article we calculated the mean temperatures and surface brightness of main galactic radio loops at 1420 MHz. We computed the mean temperatures of the major radio loops I, II, III and IV using the data taken from the northern sky radio continuum survey. We also compared our results with results obtained at other wavelengths. The results showed good agreement when reduced to 1000 MHz.en_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomska opservatorijaen_US
dc.relation.ispartofPublications of the Astronomical Observatory of Belgradeen_US
dc.titleBrightness of main galactic radio loops at 1420 MHzen_US
dc.typeConference Objecten_US
dc.relation.conferenceNational Conference of Astronomers of Serbia and Montenegro (14 ; 2005 ; Belgrade)en_US
dc.relation.publicationProceedings of the XIV National Conference of Astronomers of Serbia and Montenegro, 12-15 okt. 2005en_US
dc.identifier.urlhttps://publications.aob.rs/80/pdf/061-064.pdf-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0373-3742en_US
dc.description.rankM63en_US
dc.relation.firstpage61en_US
dc.relation.lastpage64en_US
dc.relation.issue80en_US
item.grantfulltextnone-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairetypeConference Object-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0003-0665-0939-
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