Extended Data Figure 3 : Enhancement in dust continuum emission.

From: Resolved images of a protostellar outflow driven by an extended disk wind

Extended Data Figure 3

ad, Observed radial continuum brightness profile (square data points) at the four position angles indicated in the inset at top right. ‘Position’ angle 76° corresponds to the long axis of the disk on the northeastern side where the blueshifted northern outflow is launched. A Gaussian fit is overlaid as a dashed line. eh, Residual intensity after subtracting the fits shown in the left column (square points), and a Gaussian fit (dashed line) to determine the peak location of the enhancement. The grey-filled area denotes the 2σ root-mean-square noise in the continuum map.