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Paper: Redistribution of Metals in Interacting Galaxies
Volume: 423, Galaxy Wars: Star Formation and Stellar Populations in Interacting Galaxies
Page: 355
Authors: Rupke, D.; Kewley, L.; Barnes, J.
Abstract: Recent results have shown that nuclear, gas-phase oxygen abundances are depressed in strongly interacting galaxies. We present some of the first observed radial metallicity gradients of strongly interacting galaxies, using multi-object Keck spectroscopy. Flattened gradients, and comparison to numerical simulations, confirm that lowered nuclear abundances are caused by interaction-driven gas inflows.
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