The peculiar motion of the galaxies

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1976 English Publisher:WileyJournal:Astronomische Nachrichten, volume 297, pages 309-310 (issn: 0004-6337, eissn: 1521-3994,

Authors: H. Oleak; H.‐J. Treder;

doi: 10.1002/asna.19762970614

The peculiar motion of the galaxies

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Abstract

AbstractThe result of SANDAGE and TAMMANN (1975) that the peculiar motion of the galaxies superimposed on the HUBBLE flow is probably smaller than 50 km/s shows that the kinetic energy density of the “galaxy gas” was always smaller than the energy density of radiation or matter if the galaxies were formed later than z ≈︂ 104. The galaxies possessed initial velocities 0.2 c if they orginated in the recombination area.

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