Morphology subtypes in rich galaxy cluster with intermediate concentration

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dc.contributor.authorZabolotnii, Viktor
dc.contributor.authorPanko, Olena O.
dc.contributor.authorПанько, Елена Алексеевна
dc.contributor.authorПанько, Олена Олексіївна
dc.contributor.authorKorshunov, Valerii
dc.contributor.authorYemelianov, Yaroslav
dc.date.accessioned2020-02-20T13:39:43Z
dc.date.available2020-02-20T13:39:43Z
dc.date.issued2019
dc.description.abstractThe Universe consists of many galaxy clusters which we observe on the sky. Galaxy cluster is structure that consists of many galaxies (from 10 to 1000). In our work we are looking for rich clusters (100 and more galaxies) with intermediate concentration. We used Panko classification of galaxy clusters.uk_UA
dc.identifier.citation6-th Gamow International Conference in Odessa "New trends in astrophysics, cosmology and hep after Gamow" and 19-th Gamow Summer School "Astronomy and beyond: astrophysics, cosmology, radioastronomy and astrobiology" (Ukraine, Odessa, Chernomorka, August 11-18, 2019)uk_UA
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/27253
dc.language.isoenuk_UA
dc.subjectthe Universeuk_UA
dc.subjectgalaxy clustersuk_UA
dc.subjectrich clustersuk_UA
dc.titleMorphology subtypes in rich galaxy cluster with intermediate concentrationuk_UA
dc.typeArticleuk_UA
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