Abstract
Angular momentum exchange is a driving process for the evolution of barred galaxies. Material at resonance in the bar region loses angular momentum which is taken by material at resonance in the outer disc and/or the halo. By losing angular momentum, the bar grows stronger and slows down. This evolution scenario is backed by both analytical calculations and by N-body simulations. The morphology of the bar also depends on the amount of angular momentum exchanged.
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© 2003 Springer-Verlag Berlin Heidelberg
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Athanassoula, L. (2003). Angular Momentum Redistribution and the Evolution and Morphology of Bars. In: Contopoulos, G., Voglis, N. (eds) Galaxies and Chaos. Lecture Notes in Physics, vol 626. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-45040-5_26
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DOI: https://doi.org/10.1007/978-3-540-45040-5_26
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-40470-5
Online ISBN: 978-3-540-45040-5
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