Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-19T08:47:01.486Z Has data issue: false hasContentIssue false
  • English
  • Français

Distribution of Dark Matter in Polar Ring Galaxies

Published online by Cambridge University Press:  04 August 2017

Bradley C. Whitmore ,
Douglas B. McElroy ,
François Schweizer  and
Vera C. Rubin
Bradley C. Whitmore
Affiliation:
Space Telescope Science Institute
Douglas B. McElroy
Affiliation:
Space Telescope Science Institute
François Schweizer
Affiliation:
Dept. of Terrestrial Magnetism, Carnegie Inst. of Washington
Vera C. Rubin
Affiliation:
Dept. of Terrestrial Magnetism, Carnegie Inst. of Washington

Extract

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 discovery of SO galaxies with polar rings makes it possible to directly measure the gravitational potential of a galaxy in three dimensions. Schweizer, Whitmore and Rubin (1983) find a spherical potential in the case of A0136-0801. We have observed three more polar ring galaxies using the 4 meter telescope at CTIO. The following table summarizes the results for these three systems as well as A0136-0801, and figure 1 shows an example of the data.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 117: Dark Matter in the Universe , 1987 , pp. 315
Copyright
Copyright © Reidel 1987 

References

Schweizer, , Whitmore, , and Rubin, 1983, A.J., 88, 909.Google Scholar