Fig. 9

Maser disk inner (left) and outer radius (right) versus 1.4 GHz continuum luminosity. The inner and outer radii are taken from from Kuo et al. (2011), Braatz et al. (2015), and Gao et al. (2017). The black dashed lines are linear fits to the data. The slope and intercept of the fit, as well as the correlation coefficient and the P-value of the Spearman test (see also Fig. 5) are shown in a corner of each plot.
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