Abstract
Two galaxy models are examined as illustrations of the modal approach to the problem of spiral structure. First a simple model is considered to demonstrate the effect of superposition of modes. Next a possible model for the Milky Way is shown for the purpose of exploring the effect on the unstable modes of three different rotation curves; falling, flat or rising.
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© 1983 D. Reidel Publishing Company, Dordrecht, Holland
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Haass, J. (1983). A Modal Approach to Spiral Structure: Two Examples. In: Shuter, W.L.H. (eds) Kinematics, Dynamics and Structure of the Milky Way. Astrophysics and Space Science Library, vol 100. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7060-1_39
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DOI: https://doi.org/10.1007/978-94-009-7060-1_39
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-009-7062-5
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