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Fig. 12


Radio fluxes of Cyg OB2 #5 as a function of phase in the 2366 d cycle (with tAB+C,0 = 34909) along with the best-fit model with s = 2 (see text). The crosses stand for the VLA data from Kennedy et al. (2010), whereas the filled dots indicate the VLBA fluxes from Dzib et al. (2013) multiplied by a factor 4/3 and with a 5 mJy offset added (see text). The VLBA data were not used in the fit but they nevertheless agree well with VLA results.

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