Maps of kinematic parameters. Top: gas velocity dispersion of the cloud traced using the DCO⁺ (3-2). Bottom: centroid velocity map obtained fitting the observed DCO⁺ (3-2). The black vectors represent the polarization angles, tilted by 90 degrees to trace the magnetic field direction (Redaelli et al. 2019a). The blue and red arrows show the direction of the outflow (PA = 35°, from Bjerkeli et al. 2016), and the yellow arrow presents the mean velocity gradient direction around the core. The star shows the position of the protostar. The contours represent N(H₂) column density levels, as derived from Herschel data: [1.0, 1.5, 2.0] 10²² cm⁻².