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Fig. 5


Comparison of observed H2O line profiles (in black) towards NGC 1333-IRAS 2A, 4A, and 4B by Kristensen et al. (2010) with synthetic predictions (solid red curves) for the grid model best fitting the 557 GHz line in each source with parameters listed at the bottom. Predicted profiles for a smaller = 6.4 AU are also shown for comparison (dashed green).

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