Photometric Imaging of Abell Clusters in the Aquarius Supercluster `Knot'

Details Photometric Imaging of Abell Clusters in the Aquarius Supercluster `Knot' Photometric Imaging of Abell Clusters in the Aquarius Supercluster `Knot'

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002noao.prop..360b&link_type=abstract

NOAO Proposal ID #2002B-0360

Physics

Scientific paper

We propose R and V imaging of six Abell clusters in the Aquarius Supercluster 'knot.' This is one of the four identified highest density peaks in the cluster spatial distribution. A Tully-Fisher distance determination versus redshift study of peculiar motions is expected to show whether or not this knot has broken with the Hubble flow and is now in collapse. Our imaging of these clusters will allow selection of near- edge-on spirals for our planned proposal for multi-aperture spectroscopic observations of the supercluster.

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