A search for gas-rich dwarf galaxies just outside the Local Supercluster

Astronomy and Astrophysics – Astronomy

Scientific paper

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Dwarf Galaxies, Galactic Clusters, Irregular Galaxies, Galactic Evolution, Galactic Mass, Red Shift, Star Formation

Scientific paper

Results are presented of the sampling of the nearest void in the distribution of galaxies, in a direction perpendicular to the fundamental plane of the Local Supercluster, in the neutral hydrogen spectral line for low-mass gas clouds or H I-rich dwarf galaxies. None were found, to a smaller H I mass limit than has been previously reported for a low-density region in the large-scale distribution of galaxies. An upper limit of about 5 percent of closure density in the form of gas clouds with MH of greater than about 5,000,000 solar masses is given. It is suggested that the ratio of gas-rich dwarfs to spirals is no higher in voids than in superclusters, and that dwarf irregular galaxies with MH below 10 exp 8 solar masses are less common than galaxies of greater mass. Two new members of a previously detected group of galaxies at a redshift of about 2500 km/s, representing an 'island' in the void, were detected, along with four galaxies in the background.

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