Cosmology using the Parkes Multibeam Southern-Sky HI Survey

dc.creatorThomas, P. A.
dc.date1996-07-02
dc.date.accessioned2026-07-07T02:21:26Z
dc.date.available2026-07-07T02:21:26Z
dc.descriptionI discuss the implications of the Parkes HI Multibeam Southern Sky Survey for cosmology. It will determine the local mass function of HI clouds, detecting several hundred per decade of mass. Each of these will come with a redshift and, for the more massive clouds, an estimate of the velocity width. This will provide an ideal database for peculiar motion studies and for measurements of biasing of galaxies relative to the underlying matter distribution.
dc.description10 pages including 6 figures. Full version of Figure 4 available from ftp://star.maps.susx.ac.uk/pub/papers/pat/hicol_full.ps.Z Submitted to PASA as part of the Proceedings of the Workshop on HI in the Local Universe, Sydney, 13-15 May 1996
dc.identifierhttps://arxiv.org/abs/astro-ph/9607010
dc.identifierhttp://arxiv.org/abs/astro-ph/9607010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10548
dc.subjectAstrophysics
dc.titleCosmology using the Parkes Multibeam Southern-Sky HI Survey
dc.typetext

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