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Kinematics of the LMC CH-stars
Published online by Cambridge University Press: 19 July 2016
Abstract
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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