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Fig. 3

image

Mira A and B spectral energy distribution from the radio to the submillimeter frequency range as probed by ALMA and the VLA. The round (red) symbols denote Mira A and the squares (blue) Mira B. The gray symbols are from the literature referred to in the text. The errors on the VLA data points only contain the formal flux density uncertainties, while the ALMA error bars also contain the absolute uncertainties (5% and 10% for Bands 3 and 6 together, and Band 7, respectively). The dotted lines indicate the Reid & Menten (1997) model for Mira A and the fit to the VLA data for Mira B. The dashed line at the Band-3 points is the spectral index derived within the Band, and the green dashed line is the fit to the ALMA Bands 3 and 6 data.

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