Figure 12.
Left: H i is shown with contours at 10, 50, 100, 250 and 500 (Jy beam−1)(m s−1) as seen previously in Fig. 2. The underlying grey scale shows the velocity divided by dispersion from the analysis by Hunter et al. (2012). Right: the RGB star distribution is shown in the contours (1.5, 3 and 10σ above the mean background) overlaying the H i distribution in grey-scale.
