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Paper: An HI Study of the Ursa Major Cluster of Galaxies
Volume: 240, Gas and Galaxy Evolution: A Conference in Honor of the 20th Anniversary of the VLA
Page: 573
Authors: Verheijen, M. A. W.
Abstract: The WSRT is used to obtain detailed kinematics of a complete volume limited sample of spiral galaxies in the Ursa Major Cluster, useful for studies of the Tully-Fisher relation and the properties of dark matter halos. In this short contribution, a brief overview of the global HI morphologies will be presented along with some statistics on the occurrence of tidal interactions, warps, and lopsidedness.
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