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Supernova Feedback in SPH Simulations of Galaxies
Published online by Cambridge University Press: 26 May 2016
Abstract
We report on the development of a N-body/SPH code for galaxy interactions, with particular emphasis on SN feedback implementations. We show that current methods of SN feedback probably need simulations with > 105 – 106 gas particles per galactic disk to be able to realistically describe galactic fountains and superwinds.
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- Copyright © Astronomical Society of the Pacific 2003