Fig. 1.
Gaia-2MASS diagram of LPVs in the LMC (left) and SMC (right). Boundaries between various groups of stars are defined as in Lebzelter et al. (2018), except for the redefined boundary between branches (c) and (d) (see Sect. 2.1). Boundaries of the SMC account for the different distance with adopted distance moduli 18.49 mag and 18.96 mag, respectively (de Grijs et al. 2017).
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