Confirmation of a large-scale, large-amplitude flow in the direction of the great attractor

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astronomical Spectroscopy, Elliptical Galaxies, Galactic Clusters, Spiral Galaxies, Astronomical Photometry, Dark Matter, Flow Velocity, Galactic Evolution, Radial Velocity

Scientific paper

New spectroscopy and photometry have been obtained for 136 elliptical and S0 galaxies in the direction of the large-scale streaming flow described by Dressler et al. and Lynden-Bell et al. These data are used with the Dn-sigma relation to predict distances for these galaxies, and, by comparison with their observed radial velocities, to predict their peculiar motions relative to a smooth Hubble flow. In excellent agreement with the earlier work, a gradually rising, coherent flow is found in the direction of the Hydra-Centaurus supercluster out to a distance of about 3000 km/s with an average flow velocity of about 1000 km/s with respect to the frame defined by the cosmic background radiation. The peculiar motions are then seen to decrease to near zero by a distance of about 4000 km/s. This is in general agreement with the model proposed by Lynden-Bell et al., which ascribes the flow to the gravitational pull of a 'great attractor'.

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