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dc.contributor.authorRadulović, Nikolaen_US
dc.contributor.authorPavlović, Marinaen_US
dc.contributor.authorProdanović, Tijanaen_US
dc.date.accessioned2020-12-16T11:44:29Z-
dc.date.available2020-12-16T11:44:29Z-
dc.date.issued2019-
dc.identifier.issn0352-4906-
dc.identifier.urihttp://researchrepository.mi.sanu.ac.rs/handle/123456789/4511-
dc.description.abstractIrregular galaxies are considered to be results of collisions or close approaches between galaxies. In the local universe, determining the morphological type and collision stage does not pose a problem. However, when it comes to galaxies at high redshifts, determining morphology is non-trivial. In this paper, the morphological parameters used to determine the morphology of galaxies at large redshifts will be summarised and described in detail. The aim of this research is to examine the sensitivity of morphological parameters at different collision stages on galaxies in the Local Universe, so that the most sensitive parameter can be found and later applied to the study of collisions between distant galaxies.en_US
dc.publisherMatica srpska, Novi Saden_US
dc.relation.ispartofZbornik Matice srpske za prirodne naukeen_US
dc.subjectgalaxy morphology | high redshift | morphology parametersen_US
dc.titleExamining the morphology of galaxies at high redshiftsen_US
dc.typeArticleen_US
dc.identifier.doi10.2298/ZMSPN1937023R-
dc.relation.firstpage23-
dc.relation.lastpage31-
dc.relation.volume137-
dc.description.rankM51-
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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