THE CRITERIA FOR MORPHOLOGICAL CLASSIFICATION OF PF GALAXY CLUSTERS

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dc.contributor.authorPanko, Olena O.
dc.contributor.authorПанько, Елена Алексеевна
dc.contributor.authorПанько, Олена Олексіївна
dc.date.accessioned2014-03-28T07:37:51Z
dc.date.available2014-03-28T07:37:51Z
dc.date.issued2013
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2013 . – Vol.26/1.uk
dc.description.abstractThe morphological types of galaxy clusters resulting from their outward appearance is physically related to the clusters and their member galaxies. Presented here is an adopted system of morphological types of galaxy clusters based on the Zwicky, Boutz & Morgan, Rood & Sastry, and L´opez-Cruz systems. The adopted types are suitable for automated classification of galaxy clusters from The Catalogue of Galaxy Clusters and Groups (Panko & Flin 2006). Numerical criteria describing 6 main types were distinguished: Concentrated C, Intermediate I, Open O, Line L, Flat F, and cD. The types correspond to the base divisions from regular to irregular clusters, but also note the presence of preferential direction or plane in each cluster.uk
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/4778
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;;vol. 26, issue 1, p. 90-93
dc.subjectclusters of galaxiesuk
dc.subjectmorphological typesuk
dc.titleTHE CRITERIA FOR MORPHOLOGICAL CLASSIFICATION OF PF GALAXY CLUSTERSuk
dc.typeArticleuk
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Odesa Astronomical Publications