The Transfer of Angular Momentum between Interacting Galaxies

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Scientific paper

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Galaxies: Interactions, Galaxies: Kinematics And Dynamics, Galaxies: Evolution, Methods: Numerical

Scientific paper

In this work, we employ a TREE-Code to study the collision of two spiral
galaxies when they approach each other in a parabolic orbit. During a
collision, we follow the evolution of the angular momentum (AM) of the
different components of the galaxies, i.e., disk, bulge and halo.

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