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Kinematics of the LMC CH-stars

Published online by Cambridge University Press:  19 July 2016

F.D.A. Hartwick  and
A. P. Cowley
F.D.A. Hartwick
Affiliation:
Dept. of Physics and Astronomy, University of Victoria, Victoria BC, V8W 2Y2, Canada
A. P. Cowley
Affiliation:
Dept. of Physics and Astronomy, Arizona State University Tempe, Arizona, 85287, USA

Abstract

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Velocities have been measured for 74 CH stars in the direction of the Large Magellanic Cloud (LMC). These have been used to study the kinematics of the oldest stellar population. Velocities of these objects appear to reflect two distinct subgroups - one associated with the old globular cluster population and a second with the LMC disk.

Type
Large-Scale Structure and Kinematics
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 77 - 80
Copyright
Copyright © Kluwer 1991 

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