¹²CO (J = 3−2) spectral cubes covering a 3.3′ × 3.3′ field surrounding IRAS 18345 in a velocity range 77.6 km s^-1 to 113.5 km s^-1 centred on the CO-line rest frequency. The left and right panels show the spectral cube in two different orientations. The central panel shows the same region as in the left panel, but with the faint emission filtered out to show the outflow more clearly. The red square shows the plane of the υ_LSR of the core. The contours representing the blue- and red-shifted outflow lobes projected on to the sky plane are shown in Fig. 1.