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Dark-to-luminous mass ratio in spiral galaxies

Published online by Cambridge University Press:  07 August 2017

P. Jablonka  and
N. Arimoto
P. Jablonka
Affiliation:
Observatoire de Meudon, D.A.E.C, URA 173 CNRS, 92195 Meudon, France
N. Arimoto
Affiliation:
Observatoire de Meudon, D.A.E.C, URA 173 CNRS, 92195 Meudon, France

Abstract

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We demonstrate that, contrary to the conventionnal view, late type spirals do not seem to contain more dark matter than early type ones.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 437
Copyright
Copyright © Kluwer 

References

Arimoto, N., Jablonka, P., 1991, Astron. Astrophys. in press.Google Scholar
Jablonka, P., Arimoto, N., 1991, Astron. Astrophys. in press.Google Scholar
Tinsley, B.M.: 1981, Mon. Not. Roy. Astron. Soc. 194, 63.CrossRefGoogle Scholar
Vader, J.P.: 1984, in Formation and evolution of galaxies and large scale structures in the Universe, eds. Audouze, J., Van, J.T.T., D. Reidel Publishing Compagny, p.227.CrossRefGoogle Scholar