Fig. 2

Position–velocity diagrams of HH 1042 (top) and HH 1043 (bottom) for various lines, as labeled. The absolute flux scale is logarithmic. The underlying stellar continuum (at distance = 0′′), where present, was subtracted using a Gaussian fit. The ambient cloud produces emission in most lines at zero velocity (by definition) over the full length of the slit. In most lines the blue lobe of the HH 1042 jet is very prominent, while the red lobe suffers from extinction. The measured radial velocities in HH 1043 are significantly lower than those in HH 1042.
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.