Fig. 2.
Download original image
NIRCam narrow-band images of DG Tau B: (a) F164N = continuum + [Fe II], (b) F212N = continuum + H2 1−0 S(1), (c) F323N = continuum + H2 1−0 O(5). The black star at (0, 0) marks the position of the disk continuum emission peak observed with ALMA at 232 GHz (DV20), which is considered to be the source position. The orientation on the sky is shown in panel a. The ΔZ axis points towards the redshifted jet at PA = 295°.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.