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The Pattern Speed of NGC 936 by the Tremaine-Weinberg Method

Published online by Cambridge University Press:  12 April 2016

Konrad Kuijken  and
Michael R. Merrifield
Konrad Kuijken
Affiliation:
Kapteyn Institute, PO Box 800, 9700 AV Groningen, Netherlands
Michael R. Merrifield
Affiliation:
Dept. of Physics, Southampton University, SO17 1BJ, UK

Abstract

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We describe a kinematic measurement of the pattern speed in the classic SB0 galaxy NGC 936. While the practicalities of this method remain difficult, allowance for non-Gaussian velocity distributions enables more reliable measurements than hitherto possible. The bar of NGC 936 appears to end just inside its corotation radius.

Type
Part IV. Observations of Barred Galaxies: Stellar Kinematics, Bulges, AGN
Information
International Astronomical Union Colloquium , Volume 157: Barred Galaxies , 1996 , pp. 215 - 217
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Kent, S.M. 1987, AJ, 93, 1062 CrossRefGoogle Scholar
Kormendy, J. 1984, ApJ, 286, 132 CrossRefGoogle Scholar
Merrifield, M.R. & Kuijken, K. 1995, MNRAS, 274, 933 CrossRefGoogle Scholar
Tremaine, S.D. & Weinberg, M.D. 1984, ApJ, 282, L5 CrossRefGoogle Scholar