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An HI Study of Ursa Major Spirals
Published online by Cambridge University Press: 25 May 2016
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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.
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- Copyright © Kluwer 1996