Fig. 12.
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Period–amplitude diagram of the FM (top panel) and 1OM (bottom panel) of SRVs and Miras in the LMC, colour-coded by the branch of the G2MD they belong to. Sources with uncertain chemical type are identified by diamond symbols. The dashed line in the top panel has the same meaning as in Fig. 5, i.e., it marks the assumed separation between O-rich SRV-0+ and SRV-0− stars.
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