Abstract
We describe detailed CO (2 → 1) observations of NGC 2264G. This object is a highly collimated bipolar molecular outflow that has been completely mapped with moderately high resolution as described here. We present the data as an atlas of contoured channel maps and show spectra at numerous positions of importance. We show that at several positions in the low-velocity outflow lobes, the emission from the outflow dominates the emission within the velocity range of the line core.
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