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Tully-Fisher Relations from an HI-Selected Sample
Published online by Cambridge University Press: 26 May 2016
Abstract
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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.
- Type
- Part 12: Dark and Visible Matter Scaling Relations
- Information
- Symposium - International Astronomical Union , Volume 220: Dark Matter in Galaxies , 2004 , pp. 411 - 412
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
References
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