DC FieldValueLanguage
dc.contributor.authorPavlović, Marinaen_US
dc.contributor.authorProdanović, Tijanaen_US
dc.date.accessioned2020-12-16T11:40:12Z-
dc.date.available2020-12-16T11:40:12Z-
dc.date.issued2019-
dc.identifier.issn0352-4906-
dc.identifier.urihttp://researchrepository.mi.sanu.ac.rs/handle/123456789/4510-
dc.description.abstractFar infrared-radio correlation represents a linear relationship between far-infrared (FIR) and radio emission in star-forming galaxies. Previous observations have confirmed that this correlation is maintained over a large range of redshift and does not evolve, although a small dispersion is present. However, some of more recent observations at high redshift have shown the opposite. The question that arises is - what is driving this evolution? In this paper we investigate the possibility that galaxy morphology is the answer to this question. A sample of 37 submillimeter galaxies (SMGs) is analyzed. The observation and morphological class of these galaxies has previously been published. We examined FIR-radio correlation in galaxies of different morphological type in this sample and found that for star-forming disk galaxies correlation is stable and does not evolve and for irregular and interacting galaxies we find some hints of evolution.en_US
dc.publisherMatica srpska, Novi Saden_US
dc.relation.ispartofZbornik Matice srpske za prirodne naukeen_US
dc.subjectcosmic rays | galaxy evolution | interactions of galaxies | infrared: galaxies | radio continuum: galaxiesen_US
dc.titleWhat is driving the evolution of the far-infrared radio correlation?en_US
dc.typeArticleen_US
dc.identifier.doi10.2298/ZMSPN1937009P-
dc.relation.firstpage9-
dc.relation.lastpage16-
dc.relation.volume137-
dc.description.rankМ51-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.openairetypeArticle-
item.grantfulltextnone-
crisitem.author.orcid0000-0001-5560-7051-
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