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Fig. 6.

image

Comparison between the observed flux densities (solid black circles; Osorio et al. 2017; Tobin et al. 2019) and the best-fit models (solid magenta lines) for the three knots, VLA 12N, 12C, and 12S. The grey shaded areas encompass the models within a confidence interval between 50% (second quartile) and 96% (2σ).

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