Fig. 10.
Same as Fig. 7, but for M 3. The approximate color range of the instability strip from Clementini et al. (2019) is indicated in the upper left panel by vertical dashed lines and the pulsating variable (see main text) is labeled “RRab”. We note that the illustrated color and brightness for the RR Lyrae star are merely mean quantities, which may vary substantially over the pulsation cycle.
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