Composite image (24, 100, and 160 μm) of the HD 176386/TY CrA region, with the LABOCA 870 μm contours (at 0.1, 0.2, 0.25, 0.4, and 0.7 Jy) marked in green, the 100 μm contours in black (at 0.4, 0.6, 0.8, and 1.0 Jy), and the positions of the sources as white stars. The 24 μm data trace the cavities cleared by the two massive stars. The 870 μm data reveal that the peak of the submm emission (and thus the expected higher mass column density) is located around HD 176386, but the star itself is not affected by high extinction. The Herschel data reveals a peak in the zone between the two mid-IR illuminated cavities, which could indicate the formation of condensations. To the south, some details of another submillimeter emission region that lacks far-IR sources can also be appreciated.
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.