Tully-Fisher Relations from an HI-Selected Sample

Details Tully-Fisher Relations from an HI-Selected Sample Tully-Fisher Relations from an HI-Selected Sample

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..220..411m&link_type=abstract

International Astronomical Union Symposium no. 220, held 21 - 25 July, 2003 in Sydney, Australia. Eds: S. D. Ryder, D. J. Pisano

Physics

Scientific paper

The Tully-Fisher relation is of interest because of its use as a secondary distance measure and the constraints it places on the physics of rotationally supported galaxies. We use data from the HI Parkes All-Sky Survey Catalogue to study and apply the Tully-Fisher relation on a sample of galaxies selected on their HI properties. The issues of third parameter dependencies and intrinsic scatter of the Tully-Fisher relation are investigated.

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