Arcsecond images of CH₃CN toward W75N

CH₃CN (J = 6-5) was observed with a resolution of 2″ toward W75N using the BIMA interferometer. Two continuum sources were detected at 3 mm and designated MM1 and MM2 in previous studies. Alignment of the two continuum sources with the outflow axis from MM1 suggests that these continuum sources may be the result of the outflow interacting with the interstellar medium. MM1 is coincident with compact CH₃CN emission. CH ₃CN was not detected toward MM2. The distribution of optical depth (τ_L) is derived. An excitation analysis was not done because of large-line optical depths.