The radial acceleration relation at the EDGE of galaxy formation - Testing its universality in low-mass dwarf galaxies

Open Access

Fig. 3.

Radial acceleration relation (RAR) for our sample of dwarf galaxies. Each colour corresponds to a different galaxy, where the shaded area corresponds to the 68% confidence interval and the solid line marks the median value. The dotted lines correspond to extrapolations beyond the kinematic data range. The solid black line marks the RAR derived by McGaugh et al. (2016) for SPARC local spiral galaxies. The dashed black line marks g_obs = g_bar.

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