The role of turbulence in high-mass star formation: Subsonic and transonic turbulence are ubiquitously found at early stages

Open Access

Fig. A.1

Raw data (black) and fitted model (red) of NH₃ (1,1) at the top and (2,2) at the bottom lines from the center of G48.64_c1. Fitting results are noted in the upper left corner.

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