The Adopted Morphological Types of 247 Rich PF Galaxy Clusters

dc.contributor.authorPanko, Olena O.
dc.contributor.authorBajan, Katarzyna
dc.contributor.authorFlin, Piotr
dc.contributor.authorGotsulyak, Alla
dc.contributor.authorПанько, Олена Олексіївна
dc.contributor.authorПанько, Елена Алексеевна
dc.date.accessioned2019-05-16T08:02:45Z
dc.date.available2019-05-16T08:02:45Z
dc.date.issued2016
dc.description.abstractMorphological types were determined for 247 rich galaxy clusters from the PF Catalogue of Galaxy Clusters and Groups. The adopted types are based on classical morphological schemes and consider concentration to the cluster center, the signs of preferential direction or plane in the cluster, and the positions of the brightest galaxies. It is shown that both concentration and preferential plane are significant and independent morphological criteria.uk_UA
dc.identifierdoi:10.1017/S1743921316009893
dc.identifier.citationThe Zeldovich Universe: Genesis and Growth of the Cosmic Web, Proceedings of the International Astronomical Union, IAU Symposiumuk_UA
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/24041
dc.language.isoenuk_UA
dc.relation.ispartofseries;Vol. 308.
dc.subjectGalaxiesuk_UA
dc.subjectclustersuk_UA
dc.subjectmorphological typesuk_UA
dc.titleThe Adopted Morphological Types of 247 Rich PF Galaxy Clustersuk_UA
dc.typeArticleuk_UA
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