P. A. Thomas, PASA, 14 (1), 25.
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Conclusions
- The Parkes HI Multibeam Southern Sky Survey will determine the mass function of HI clouds in the local Universe. This will provide a strong constraint on models of galaxy formation.
- The spatial distribution of HI clouds of differing mass will test ideas about biasing in the galaxy distribution.
- A complete survey of high-mass galaxies, plus Tully-Fisher estimates of distances and hence peculiar velocities, will provide strong constraints on the density parameter.
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