Colours and HI line observations in Virgo (Sabatini+, 2005)

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Clusters: Galaxy, Galaxies: Photometry, H I Data

Scientific paper

The optical data that we use in this paper are part of the 2.5-m Isaac Newton Telescope Wide Field Camera (INT WFC) survey of the Virgo Cluster (see paper I, Sabatini et al., 2003MNRAS.341..981S, for further details). Here we present results from the west-east B- and i-band strip in the cluster, extending from the centre of the cluster (identified as M87) eastwards for 7{deg}, with a total area of 14deg2. This region of the cluster is part of the dynamical unit named cluster A (M87), excluding members of other units like cluster B, clouds M and W.
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