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Frommert, Hartmut; Mayers, Kenneth; Gingerich, Owen; Holmberg, Gustav; Šolc, Martin; Saladyga, Michael; Taibi, Richard J.; Marché, Jordan D.; Hatch, Robert Alan; Blaauw, Adriaan; Elliott, Ian; Trimble, Virginia; Schnell, Anneliese; Cunningham, Clifford J.; Dialetis, Dimitris; Dumont, Simone; McMahon, John M.

doi:10.1007/978-0-387-30400-7_1044

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Application To the Lg And Virgo Cluster1

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2019

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“…With account of it the LG is moving from VC at velocity v LV ∼ 750 km/s. The behaviour of the Local Group in future was predicted in different papers [20][21][22] as follows, see also Ref. 23 "Analysis of the dynamics of the Local Supercluster has provided a picture of how the enormous mass of the Virgo Cluster acts gravitationally on the galaxies and galaxy groups around it.…”

Section: Application To the Lg And Virgo Clustermentioning

confidence: 99%

Two-body problem in presence of cosmological constant

Бисноватый-Коган

Merafina

2019

Int. J. Mod. Phys. D

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We consider the Kepler two-body problem in presence of the cosmological constant Λ. Contrary to the classical case, where finite solutions exist for any angular momentum of the system L, in presence of Λ finite solutions exist only in the interval 0 < L < L lim (Λ). The qualitative picture of the two-body motion is described, and critical parameters of the problem are found. Application are made to the relative motion of the Local Group and Virgo cluster.

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