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Anisotropy in the Hubble relation for the brightest galaxies in clusters
Authors:B. N. G. Guthrie
Affiliation:(1) Royal Observatory, Edinburgh, Scotland
Abstract:The sky distribution of deviations from the mean Hubble relation for the brightest galaxies in clusters is non-random for the velocity range 4000<Vr<25 000 km s–1. Deviations in visual magnitude are mainly positive in one large region of the sky and mainly negative in another region; the difference between the regions is 0.37±0.08m and is independent of colour. Various explanations are discussed briefly, and galactic or intergalactic absorption may be excluded.
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