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Date and Time of the Query: 2019-05-21 T00:04:09 PDT
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For refcode 1993ApJ...403L..59A:
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Copyright by American Astronomical Society. Reproduced by permission
1993ApJ...403L..59A DO ROTATION CURVES OF SPIRAL GALAXIES IN CLUSTERS DECLINE? P. AMRAM, W. T. SULLIVAN III, C. BALKOWSKI, M. MARCELIN, AND V. CAYATTE Received 1992 June 15; accepted 1992 November 12 ABSTRACT Rotation curves for 21 spiral galaxies in five clusters have been obtained in a search for possible effects of the cluster environment on individual galaxy dynamics. We find no significant evidence for anything more than a small influence of the cluster environment. In particular, using 12 selected galaxies we do not confirm the strong correlation between slope of rotation curve and location within a cluster reported by Whitmore, Fobes, & Rubin. Subject headings: galaxies: clustering - galaxies: kinematics and dynamics
Retrieve 26 NED objects in this reference.
Please click here for ADS abstract

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