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Disk Rotation Curves in Triaxial Potentials
Published online by Cambridge University Press: 04 August 2017
Abstract
The apparent rotation curve of cold gas in a triaxial potential often differs from that in an axisymmetric system in characteristic ways. The data argue for triaxial bulges in our Galaxy and several others.
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- Information
- Symposium - International Astronomical Union , Volume 127: Structure and Dynamics of Elliptical Galaxies , 1987 , pp. 399 - 400
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- Copyright © Reidel 1987