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Dark Matter in the Polar Ring Spiral NGC 660

Published online by Cambridge University Press:  07 August 2017

Wim Van Driel
Wim Van Driel*
Affiliation:
Nançay Radio Observatory, Observatory of Paris-Meudon, 92195 Meudon, France

Extract

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Polar ring galaxies, where rotation velocities can be measured in two orthogonal planes, are generally considered to be ideal objects for studies of the three-dimensional distribution of dark matter in galaxies.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 164: Stellar Populations , 1995 , pp. 435
Copyright
Copyright © Kluwer 1995 

References

Combes, F., Braine, J., Casoli, F., Gerin, M. and van Driel, W. (1992), Molecular Gas in a Polar Ring, A&A, 259, L65 Google Scholar
van Driel, W., Combes, F., Casoli, F., Gerin, M., Nakai, N., Miyaji, T., Hamabe, M., Sofue, Y., Ichikawa, T., Yoshida, S., Kobayashi, Y., Arimoto, N., Geng, F., Kodama, T., Minezaki, T. Goudfrooij, P., Mulder, P. S., Wakamatsu, K. and Yanagisawa, K. (1994), The Polar Ring Spiral Galaxy NGC 660, A.J., in press Google Scholar