Oxygen- and carbon-rich variable red giant populations in the Magellanic Clouds from EROS, OGLE, MACHO, and 2MASS photometry

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Fig. 10

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Separation of C-rich, O-rich AGB, and red variables below the TRGB for LMC from OGLE LPV I and V photometry (Soszynski et al. 2005). The colour slope parameter a_V vs. the amplitude of colour change (left panel). The colour slope parameter a_V vs. K 2MASS magnitude (middle panel). Colour slope parameter vs. J − K colour (right panel).

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