An HI Study of the Ursa Major Cluster of Galaxies

OnderzoeksoutputAcademicpeer review

Samenvatting

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.
Originele taal-2English
Titel Gas and Galaxy Evolution
SubtitelASP Conference Proceedings
RedacteurenJohn E. Hibbard, Jacqueline H. van Gorkom
UitgeverijAstronomical Society of the Pacific
Pagina's573
ISBN van geprinte versie1-58381-077-3
StatusPublished - 2001
Extern gepubliceerdJa

Publicatie series

NaamASP Conference Proceedings
Volume240

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