Fig. 5.
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Upper panel: MK, 0 LFs of Tc-rich, M/MS-type Miras from Uttenthaler et al. (2019, solid line), and M-type Miras with bumps in their light curves (dashed line). Lower panel: MK, 0 LFs of Tc-poor, M-type Miras (solid line), and M-type Miras without bumps in their light curves (dashed line). The mean MK, 0 magnitude and the standard deviation of each group are reported in the legend.
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