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The Shape of the Disk: Clues from the Kinematics of Disk Stars
Published online by Cambridge University Press: 25 May 2016
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It is a tall task to determine the structural parameters of one's own galaxy much less any deviations from axisymmetry. Nonetheless, after hard work, the existence of asymmetries has been reported and discussed in the literature from a wide variety of sources (most recently, Nakai & Nishiyana 1994). Now, in order to understand Milky Way evolutionary history, it is our job to determine the origin and intrinsic structure of these asymmetries.
- Type
- Chapter 1: Are the Disk and Halo Axisymmetric?
- Information
- Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 11 - 21
- Copyright
- Copyright © Kluwer 1996
References
Nakai, and Nishiyana,
1994,
Radial Distributions of Hα in Barred Galaxies, M83, NGC 4321, NGC 1365, and the Galaxy
, preprint.Google Scholar
Schechter, P. L., Aaronson, M., Blanco, V. M., and Cook, K. H.
1987, in Blitz, L. and Lockman, J. (eds.),
The Outer Galaxy
, pp 31–39, Springer-Verlag.Google Scholar
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