Fig. 6

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Difference between the velocity components of each fiber in NGC 1333 SE, as recognized after the clustering. Left: resulting difference after subtracting the N2H+ υLSR from the HC3N υLSR of the clusters belonging to the redshifted fiber. Middle: resulting difference after subtracting the N2H+ υLSR from the HC3N υLSR of the clusters belonging to the blueshifted fiber. The blueshifted fiber map is zoomed into the region covered by the emission. Right: 2D KDE of the HC3N υLSR vs. N2H+ υLSR. The dotted line represents the location where the velocities are equal, and the dash-dotted line shows where the HC3N υLSR is higher by 0.11 km s−1 (the median difference for the redshifted fiber).
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