Abstract:Understanding quenching mechanisms in low-mass galaxies is essential for understanding galaxy evolution overall. In particular, isolated galaxies are important tools to help disentangle the complex internal and external processes that impact star formation. Comparisons between quenched field and satellite galaxies in the low mass regime offer a substantial opportunity for discovery, although very few quenched galaxies with masses below π β βΌ10 9 π are known outside the virial radius, π π£ππ , of any host … Show more
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