Radio outburst from a massive (proto)star - II. A portrait in space and time of the expanding radio jet from S255IR NIRS 3

Open Access

Fig. 13

Lower limit on the opening angle estimated from Eq. (10) for all the epochs of our monitoring. The bars indicate the standard deviation of the values obtained in the different bands. The dashed line connects the values of θ₀ obtained from the best fits to the spectra (see Table 6).

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