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Parameters of the Dark Halo distribution around M 31

Published online by Cambridge University Press:  12 April 2016

P. Tenjes
Affiliation:
Tartu Observatory, Tõravere, 61602, Estonia
J. Einasto
Affiliation:
Tartu Observatory, Tõravere, 61602, Estonia

Abstract

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Available observational data allow us to discriminate between the visible matter and the dark matter in M 31 and thus to determine the most important parameters of the dark halo (the mass, the radius and the outer extent).

Type
Part 5. Dark Matter and Clustering
Copyright
Copyright © Astronomical Society of the Pacific 2000

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