Hostname: page-component-cc8bf7c57-5wl6q Total loading time: 0 Render date: 2024-12-12T04:41:18.416Z Has data issue: false hasContentIssue false

The Nature of High HI Mass-to-Light Ratio Galaxies

Published online by Cambridge University Press:  26 May 2016

Bradley E. Warren
Affiliation:
Research School of Astronomy and Astrophysics, ANU, Mount Stromlo Observatory, Cotter Road, Weston ACT 2611, Australia
Helmut Jerjen
Affiliation:
Research School of Astronomy and Astrophysics, ANU, Mount Stromlo Observatory, Cotter Road, Weston ACT 2611, Australia
Bärbel S. Koribalski
Affiliation:
ATNF, CSIRO, PO Box 76, Epping NSW 1710, Australia

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.

We present here preliminary results of our multi-wavelength investigation into high HI mass-to-light ratio dwarf galaxies identified in the HIPASS Bright Galaxy Catalog.

Type
Part 1. Census
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Karachentsev, I. & Musella, I. 1996, A&A, 315, 348.Google Scholar
Koribalski, B., et al. 2003, AJ (submitted).Google Scholar
Paturel, G., et al. 1997, A&AS, 124, 109.Google Scholar
Schlegel, D.J., Finkbeiner, D.P., Davis, M. 1998, ApJ, 500, 525.Google Scholar
van Zee, L., Haynes, M.P., & Giovanelli, R. 1995, AJ, 109, 990.Google Scholar