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Fig. 12.
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Observed emission (black) of H2 S(5) (left), S(2) (middle) and S(1) (right) and the expected profiles (red), for which we assume the presence of a molecular outflow with similar kinematic properties and relative flux contribution as in the MIR H2 lines. The troughs at the peak of the S(2) and S(1) are due to the noise.
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