Abstract
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.
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© 1996 Springer Science+Business Media Dordrecht
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Verheijen, M.A.W. (1996). An HI Study of URSA Major Spirals. In: Bender, R., Davies, R.L. (eds) New Light on Galaxy Evolution. International Astronomical Union / Union Astronomique Internationale, vol 171. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0229-9_173
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DOI: https://doi.org/10.1007/978-94-009-0229-9_173
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-3976-2
Online ISBN: 978-94-009-0229-9
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