DYNAMICAL FRICTION IN THE LOCAL GROUP

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dc.contributor.authorKudinova, A. V.
dc.date.accessioned2014-03-29T02:22:12Z
dc.date.available2014-03-29T02:22:12Z
dc.date.issued2013
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2013 . – Vol.26/2uk
dc.description.abstractIn this paper we consider dynamical behavior of the astrophysical objects in the Local Group. The motion of Andromed and The Milky Way is studied. We distinguish two different models: for the first one we do not take into account the influence of the Intra-Group Matter (IGrM), for the second one we take into account the dynamical friction due to the IGrM. We obtained some characteristic IGrM parametres such as particle masses for principle cases of the collision between the giant galaxies and the situation when the merger becomes problematic. We also define the region in the vicinity of our Local Group where the formation of the Hubble Flows starts.uk
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/4790
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;vol. 26, issue 2, p. 197-200
dc.subjectLocal groupuk
dc.subjectHubble flowsuk
dc.subjectGalaxiesuk
dc.subjectMilky Wayuk
dc.subjectAndromedauk
dc.titleDYNAMICAL FRICTION IN THE LOCAL GROUPuk
dc.typeArticleuk
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Odesa Astronomical Publications