@inproceedings{26cc9c9d653b425ca03441b2fec5d077,
title = "An HI Study of the Ursa Major Cluster of Galaxies",
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.",
author = "Verheijen, {M. A. W.}",
year = "2001",
language = "English",
isbn = "1-58381-077-3",
series = "ASP Conference Proceedings",
publisher = "Astronomical Society of the Pacific",
pages = "573",
editor = "Hibbard, {John E. } and { van Gorkom}, {Jacqueline H.}",
booktitle = "Gas and Galaxy Evolution",
}