Fig. 11.
ALMA image of the red supergiant star Wd1-26 shown in colour-scale. Contours are plotted at −1, 1, 1.41, 2, 2.83, 4, 5.66, 8, 11.31, 16 × 3σ where σ is 64 μ Jy beam−1. See Appendix B for further images of W26 comparing the mm emission with that seen in the 8.6 GHz radio emission from Do10 and the Hα images presented by Wright et al. (2014).
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