tokens: We thank William Gray, Christopher Matzner, Prateek Sharma, and Robert Thacker for helpful discussions and the anonymous referee for comments. S.S. and E.S. were supported by the National Science Foundation grant AST11-03608 and NASA theory grants NNX09AD106 and NNX15AK82G. E.S. gratefully acknowledges the Simons Foundation for funding the workshop Galactic Winds: Beyond Phenomenology which helped to inspire this work. He also gratefully acknowledges Joanne Cohn, Eliot Quataert, and the UC Berkeley Theoretical Astronomy Center, and Uroš Seljak and the Lawrence Berkeley National Lab Cosmology group for hosting him during the period when much of this work was carried out. Part of this research was carried out during the visit of E.S. and E.C.O. at the KITP in UC Santa Barbara, which is supported by the National Science Foundation under grant PHY-1125915. The work of E.C.O. on this project was supported by the National Science Foundation under grant AST-1312006. The authors thank the Texas Advanced Computing Center (TACC) at The University of Texas at Austin (URL: http://www.tacc.utexas.edu ) and the Extreme Science and Engineering Discovery Environment (XSEDE) for providing HPC resources via grant TG-AST140004 that have contributed to the results reported within this paper. The FLASH code is developed in part by the DOE-supported Alliances Center for Astrophysical Thermonuclear Flashes (ASC) at the University of Chicago.
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