Hostname: page-component-76fb5796d-2lccl Total loading time: 0 Render date: 2024-04-25T21:54:01.435Z Has data issue: false hasContentIssue false
  • English
  • Français

Tully-Fisher Relations from an HI-Selected Sample

Published online by Cambridge University Press:  26 May 2016

Martin J. Meyer ,
Martin A. Zwaan ,
Rachel L. Webster  and
Stephen E. Schneider
Martin J. Meyer
Affiliation:
School of Physics, University of Melbourne, VIC 3010, Australia
Martin A. Zwaan
Affiliation:
School of Physics, University of Melbourne, VIC 3010, Australia
Rachel L. Webster
Affiliation:
School of Physics, University of Melbourne, VIC 3010, Australia
Stephen E. Schneider
Affiliation:
Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Jarrett, T. H., Chester, T., Cutri, R., Schneider, S., Skrutskie, M., & Huchra, J. P. 2000, AJ, 119, 2498.CrossRefGoogle Scholar
Meyer, M.J., Zwaan, M.A., Webster, R.L., Staveley-Smith, L., et al. 2003, MNRAS, submitted.Google Scholar