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Fig. 20

image

NH3 (1, 1) hyperfine anomaly of G351.14+0.77, which is illustrated in the upper panel, indicates a systematic outflow in this source. The middle panel displays the NH3 (1, 1) line profile of G329.180.32, which indicates an infall. This is also supported by its HNC (1–0) line in the lowest panel with a stronger blue- than redshifted peak. The source velocity is shown by the straight red line.

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