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Fig. 5.

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Kinematic support in LEWIS sample. Projected specific angular momentum (λR) as a function of galaxy ellipticity (left panel) and stellar mass (right panel). The light blue circles mark the LEWIS galaxies, and the pink squares represent the dwarf galaxies studied by Scott et al. (2020). The black curve in the left panel ( λ R = 0.31 ϵ ) $ \lambda_{\mathrm{R}}=0.31\sqrt{\epsilon}) $ splits the galaxies into rotation-supported (above the line) and dispersion-supported (below the line) systems (Emsellem et al. 2011).

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