View of the CH₃OH maser features detected around G69.52-0.97 (Table A.4). Same symbols as in Fig. 1. The polarization fraction is in the range P_l = 1.3–1.5% (Table A.5). The assumed velocity of the YSO is km s⁻¹ (Bronfman et al. 1996). The dashed line is the best least-squares linear fit of the CH₃OH maser features (°).The two arrowsindicate the direction and not the actual position of the red- and blueshifted lobes of the outflow (°, Kumar et al. 2004).