Gemini 11.7 μm continuum image (orange) from Smith et al. (2005) overlaid with SMA maps of the submillimeter continuum emission (faint white contours), the CH₃OH(7_4,3–6_4,3) A⁻ (ν_t = 1) and HC₃N(37 − 36)(ν₇ = 1) integrated emission (blue and green contours, respectively) and the rotational integrated emission of CH₃CN(12₃–11₃) (single grey contour) toward the Orion KL region. The white contours are from 40% to 90% with steps of 5% of the peak of the continuum emission (4.5 Jy beam^-1). The blue contours are from 30% to 90% with steps of 10% of the peak of the line emission, 37 Jy beam^-1 km s^-1. The integrated velocity range of the CH₃OH(7_4,3–6_4,3) A⁻ (ν_t = 2) is from  − 5 to  + 15 km s^-1. The green contours are from 25% to 90% with steps of 12% of the peak of the line emission (170 Jy beam^-1 km s^-1). The integrated velocity range of HC₃N(37 − 36)(ν₇ = 1) is from  − 12 to  + 19 km s^-1. The single grey contour is 34% of the peak of the line emission (586 Jy beam^-1 km s^-1). The integrated velocity range of CH₃CN(12₃–11₃) is from  − 10 to  + 26 km s^-1. Black circles and pink square as in previous figures. The blue and red arrows at the position of source I show the approximate orientation of the thermal and SiO maser outflow emanating from this object (Plambeck et al. 2009; Matthews et al. 2010). The white open circle marks the position of the radio source D (Zapata et al. 2004; Gómez et al. 2005).