(Re)mind the gap: A hiatus in star formation history unveiled by APOGEE DR17

Open Access

Fig. 3

Same as the upper panels of Fig. 1, but for APOGEE DR17 stars with guiding radii, R_g, between 7 and 9 kpc (we did not impose a condition on the Galactocentric distance as we did for Fig. 1) and a vertical height of |z| < 2 kpc.

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