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Fig. 4


Spatial profiles of the emission from Fig. 3 along the eastern lobe of HH 211 (top) and southern lobe of Cepheus E (bottom). The blue lines represent the 1670 GHz H2O emission, the green lines represent H2-dominated IRAC1 emission, and the red lines correspond to CO(2−1). All data have a similar resolution of approximately 13′′.

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