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An HI Study of Ursa Major Spirals

Published online by Cambridge University Press:  25 May 2016

M.A.W. Verheijen
M.A.W. Verheijen*
Affiliation:
Kapteyn Institute, Postbus 800, 9700 AV Groningen, The Netherlands

Extract

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We investigate the scatter in the TF-relations and study the Dark Matter component of spiral galaxies as a function of luminosity, morphology, scale length etc. by means of a detailed kinematic and photometric study of individual galaxies in a cluster. Because all the galaxies are at the same distance there is no doubt about their relative masses and luminosities.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 462
Copyright
Copyright © Kluwer 1996 

References

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