Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/5895
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dc.contributor.authorPanko, Olena O.-
dc.contributor.authorAndrievskii, Alexander M.-
dc.contributor.authorGotsulyak, A. V.-
dc.contributor.authorАндрієвський, Олександр Михайловичuk
dc.contributor.authorПанько, Елена Алексеевна-
dc.contributor.authorПанько, Олена Олексіївна-
dc.date.accessioned2015-02-23T12:32:28Z-
dc.date.available2015-02-23T12:32:28Z-
dc.date.issued2014-
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttp://dspace.onu.edu.ua:8080/handle/123456789/5895-
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2014 . – Vol.27, I. 1.uk
dc.description.abstractWe determined the morphological types for 254 rich galaxy clusters from the PF Catalogue of Galaxy Clusters and Groups. The data get contains the PF galaxy clusters, which have no ACO coinciding ones. The applied morphological scheme was combined of the prevalent classifications, such as Bautz-Morgan, Rood-Sastry etc approaches. We assigned the morphological types using numerical criteria and taking into consideration concentration to the cluster center, the signs of preferential direction or plane in the cluster, and the positions of the brightest galaxies. The features of the data set are discussed.uk
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;V. 27, I. 1, P. 30-31.-
dc.subjectGalaxiesuk
dc.subjectclustersuk
dc.subjectmorphological typesuk
dc.titleMorphological types of 254 Rich PF Galaxy Clustersuk
dc.typeArticleuk
Appears in Collections:Odessa Astronomical Publications

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