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Abstract

Using new HI spectral line imaging from the Very Large Array, I examine low-mass galaxies NGC 5238 and DDO 68. These are two unique dwarf galaxies with disturbed stellar morphology suggestive of a history of interaction events. I present an in-depth analysis of their HI kinematics, comparing gaseous and stellar structures, as well as a synthesis of the results of simulations constrained with these new HI data. I find that both galaxies have a highly disturbed gaseous structure that can be well explained through a history of mergers, making NGC 5238 and DDO 68 flagship examples of hierarchical assembly on the smallest of scales.

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