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Simulating galactic outflows with thermal supernova feedback
Monthly Notices of the Royal Astronomical Society, no. 1 (2012): 140-158
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摘要
Cosmological simulations make use of sub-grid recipes for the implementation of galactic winds driven by massive stars because direct injection of supernova energy in thermal form leads to strong radiative losses, rendering the feedback inefficient. We argue that the main cause of the catastrophic cooling is a mismatch between the mass of...更多
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