Fig. 3: The individual V(v) profiles for the HINSA, CNM and WNM components.
From: An early transition to magnetic supercriticality in star formation
In each panel, the red profile represents the fitted Zeeman profile of the component and the black profile represents the observed V(v) subtracted by the fitted Zeeman profiles of the other four components. The CNM and WNM Zeeman profiles include the absorption from the CNM components that lie in front but do not include the absorption from the HINSA. The sum of the red profiles of the five components is the black dashed profile in Fig. 2b.
