A Dance Of Fire And Ice: Galaxy Collapse Download

This paper examines the dual-phase collapse of a dwarf starburst galaxy, where gravitational infall triggers simultaneous extreme star formation ("fire") and the expulsion of cold molecular gas via supernovae-driven winds ("ice"). Using N-body/SPH simulations, we model the thermal and dynamical feedback loop leading to rapid quenching. Our results suggest a cyclical "dance" between heating and cooling phases that dictates the final morphology of the collapsed remnant.

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