Fig. 4
Comparisons of the integrated hyperfine intensity anomalies (inner satellites: blue dots; outer satellites: red dots) with the para-NH3 column density (a), kinetic temperature (b), velocity dispersion (c), non-thermal velocity dispersion (d), and total optical depth of NH3 (1,1) (e) all derived from the GBT NH3 observations(Friesen et al. 2017).
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