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J/MNRAS/357/819 Colours and HI line observations in Virgo LSB (Sabatini+, 2005)
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Beginning of ReadMe :J/MNRAS/357/819 Colours and HI line observations in Virgo (Sabatini+, 2005)
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The dwarf low surface brightness galaxy population of the Virgo Cluster -
II. Colours and HI line observations.
Sabatini S., Davies J., Van Driel W., Baes M., Roberts S., Smith R.,
Linder S., O'neil K.
<Mon. Not. R. Astron. Soc., 357, 819-833 (2005)>
=2005MNRAS.357..819S
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ADC_Keywords: Clusters, galaxy ; Galaxies, photometry ; H I data
Keywords: galaxies: clusters: individual: Virgo Cluster - galaxies: dwarf
Abstract:
In order to investigate the nature of dwarf low surface brightness
(LSB) galaxies we have undertaken a deep B- and I-band CCD survey of a
14-deg^2^ strip in the Virgo Cluster and applied a Fourier convolution
technique to explore its dwarf galaxy population down to a central
surface brightness of 26Bmag/arcsec^2^ and a total absolute B
magnitude of -10. In this paper we carry out an analysis of their
morphology, (B-I) colours and atomic hydrogen content.
Description:
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 7deg, with a total area of
14deg^2^. 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.