Fig. 18
Non-thermal velocity dispersions in the narrow component for each core, shell-1, and shell-2 as a function of their equivalent radii. The grey lines show the power-law fits for the range of parameters obtained from a MCMC fit, and the black line shows the best-fit model. The blue line shows the turbulence–size relation from Caselli & Myers (1995) for low-mass cores.
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