Close-up of the [C II]  map of the globule with the peak line velocity in color, determined from a Gaussian fit to each spectrum. From each Gaussian fit, the excess emission in the blue (~4 to 7 km s^-1) and redshifted (~9.5 to 11 km s^-1) wing was determined and is plotted as blue and red contours (for better visibility the maps are resampled on a finer grid). The black triangles indicate the cluster members within the H II-region (note that this is where the hot gas, visible in CO J = 11 → 10 emission is found). The gray triangles mark the three sources from the secondary cluster.