View of the CH3OH maser features detected around IRAS 22272+6358A (Table A.2). Same symbols as in Fig. 2. The assumed velocity of the YSO is Vlsr = −11 km s-1 (Beltrán et al. 2006). The two arrows indicate the direction of the red- and blue-shifted lobe of the bipolar outflow (PAout = 140°; Beltrán et al. 2006). The dashed line is the best linear fit of the CH3OH maser features (PACH3OH = 145° ± 11°).
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