Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/3934
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dc.contributor.authorEingorn, Maxim-
dc.contributor.authorZhuk, Alexander-
dc.date.accessioned2013-11-22T09:39:34Z-
dc.date.available2013-11-22T09:39:34Z-
dc.date.issued2012-
dc.identifier.citation12-th international astronomical Gamov conference-schooluk
dc.identifier.urihttp://dspace.onu.edu.ua:8080/handle/123456789/3934-
dc.description12-th Odessa International astronomical Gamow conference-school, "Astronomy and beyond: astrophysics, cosmology and gravitation, cosmomicrophysics, radio-astronomy and astrobiology" : program and abstracts, August 20-26, 2012 / "Astronomy and beyond: astrophysics, cosmology and gravitation, cosmomicrophysics, radio-astronomy and astrobiology", international astronomical Gamow conference-school (12;2012; Odessa) - ; chief I. N. Koval . – Odessa, 2012 . – 53 p.uk
dc.description.abstractWe consider the Universe deep inside of (he cell of uniformity. At these scales, the Universe is tilled with inhomogeneousiy distributed discrete structures (such as galaxies, their groups and clusters). These inhomogeneities perturb the homogeneous background, described satisfactorily by the Friedmann mode.uk
dc.language.isoenuk
dc.publisherОдеський національний університет імені І. І. Мечниковаuk
dc.subjectgravitating sourcesuk
dc.subjectcosmological expansionuk
dc.titleHubble flows and gravitational potentials in observable Universeuk
dc.typeArticleuk
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