arXiv · astro-ph/0302521
Angular momentum redistribution and the evolution and morphology of bars
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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E. Athanassoula. 2003-02-25. Angular momentum redistribution and the evolution and morphology of bars. https://doi.org/10.1007/978-3-540-45040-5_26
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