Fig. 3
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Histograms showing the distributions of the best-fit solution SED modelling parameters. From left to right: stellar effective temperature, dust inner radius temperature, density power-law index, dust shell radial optical depth at 550 nm. White bins represent ‘naked’ O-rich uvAGBs, grey bins represent O-rich uvAGBs with dust component, and striped bins represent C-rich uvAGBs.
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