The Transfer of Angular Momentum between Interacting Galaxies

Details The Transfer of Angular Momentum between Interacting Galaxies The Transfer of Angular Momentum between Interacting Galaxies

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17..101g&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Other

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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