A NEW METHOD OF STUDYING GALAXY VELOCITY FIELD: FIRST RESULTS

Details A NEW METHOD OF STUDYING GALAXY VELOCITY FIELD: FIRST RESULTS A NEW METHOD OF STUDYING GALAXY VELOCITY FIELD: FIRST RESULTS

1995-03-29

arxiv.org/abs/astro-ph/9503108v1

Astronomy and Astrophysics

Astrophysics

MNRAS submitted, 11 pages, uuencoded compressed Postscript file, including 7 figures. Postscript also available at anonymous

Scientific paper

It is shown that the average magnitude - redshift diagram for a magnitude-limited sample of galaxies can be effectively used for mapping galaxy velocity field. This new approach is quantitatively introduced and applied to the CfA, ESO/LV and ZCAT samples of galaxies. Strong arguments are presented for infall velocities in the Virgo and Fornax superclusters and in the Great Wall structure.

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