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- W1649163008 abstract "In spite of the promise of new techniques for constraining the mass distribution in galaxy clusters, much remains to be learned from galaxy orbital velocities. This article reviews the theory of potential estimation in hot dynamical systems like galaxy clusters. An analysis is presented of the Coma cluster, based on a sample of about 1500 galaxies with probable membership, of which 450 have measured velocities. We find no significant evidence for a core in either the galaxy number densities or the mass distribution." @default.
- W1649163008 created "2016-06-24" @default.
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- W1649163008 date "1995-10-18" @default.
- W1649163008 modified "2023-09-27" @default.
- W1649163008 title "Cluster Dynamics and Cluster Masses" @default.
- W1649163008 hasPublicationYear "1995" @default.
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