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tokens: ACKNOWLEDGEMENTS Our anonymous referee provided valuable feedback that helped improve this manuscript. We thank Hiroyuki Hirashita for providing us with the tabulated form of grain velocities calculated over an extended grain-size range and used in Hirashita Yan ( 2009 ). We also thank Takaya Nozawa for making available the tabulated versions of the SN grain-size distributions presented in Nozawa et al. ( 2007 ) and the SN dust destruction efficiencies used in Asano et al. ( 2013b ). Finally, we are grateful to Volker Springel for sharing access to arepo . The simulations were performed on the joint MIT-Harvard computing cluster supported by MKI and FAS. RM acknowledges support from the DOE CSGF under grant number DE-FG02-97ER25308. MV acknowledges support through an MIT RSC award and the support of the Alfred P. Sloan Foundation. PT acknowledges support from NASA through Hubble Fellowship grant HST -HF2-51341.001-A awarded by STScI, which is operated under contract NAS5-26555. RK acknowledges support from NASA through Einstein Postdoctoral Fellowship grant number PF7-180163 awarded by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for NASA under contract NAS8-03060.