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

Open Access

Fig. 1.

Stellar mass, M_★, against the half-light radius, r_1/2, for our galaxy sample. The circles indicate the classical dSphs, and the triangles represent the dwarfs from MUSE-Faint. Objects are colour-coded by the number of stars with velocities available for each object. The red stars represent the EDGE simulated dwarfs.

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