Free Access

Fig. A.7


Comparison of H13CN spectra averaged over pixels where has 5σ emission at a) Oph/main; b) Oph/cold; c) Aquila/W40; d) Aquila/Serp. South; e) Aquila/cold; f) NGC 2023; g) NGC 2024; h) NGC 2068; and i) NGC 2071. For Oph/cold, Aquila/cold, and NGC 2023, the H13CN emission is not detected. Thus, we show the spectra averaged over observing area.

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.