ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT) - VII. The layered molecular outflow from HL Tau and its relationship with the ringed disk

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Fig. 11

Footpoint radii r₀ of the B1a, B1b, and B2 shells determined from Eq. (3) at increasing offset from the source (see Table 1). The solid and dashed lines indicate the position of rings and gaps, respectively, in the continuum emission of the outer region of the disk (ALMA Partnership 2015; Stephens et al. 2023).

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