Fig. 5
MIPS 24 μm image of the area to the southeast of the giant star-forming region NGC 346 with the bow shock-producing star AzV 242 (indicated by a solid circle) and its possible parent association DEM S 118 (shown by a dashed ellipse). The arrow shows the direction of motion of the star, as suggested by the geometry of the bow shock.
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.