Applying Cosmo-topology: Galaxy Transverse Velocities

Details Applying Cosmo-topology: Galaxy Transverse Velocities Applying Cosmo-topology: Galaxy Transverse Velocities

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ctp98proce..14b&link_type=abstract

Cosmological Topology in Paris 1998, 14 December 1998, Observatoire de Paris, Eds.: V. Blanloeil, B.F. Roukema, meeting abstract

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The study of the kinematics of galaxies within clusters or groups has the limitation that only one of the three velocity components and only two of the three spatial components of a galaxy position in six-dimensional phase space can normally be measured. However, if multiple topological images of a cluster exist, then the radial positions and sky plane mean velocities of galaxies in the cluster may also be measurable from photometry of the two cluster images. ------- End of Forwarded Message

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