 | This movie shows the gas distribution of two spiral galaxies as they interact and merge. The stellar disk and the dark matter halos are included in the simulation, but are not shown. The movie spans several billion years and the frame is 50 kilo parsecs across. Interactions drive disk instabilities that funnel gas to the center. The merger remnant, a spehroidal galaxy, undergoes enhanced star formation at its center. The remaining gas forms a circumnuclear disk, a feature often observed at the center of elliptical galaxies.
Richard Plotkin, Greg Stinson
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