Importance of source structure on complex organics emission - II. Do disks explain lack of methanol emission from low-mass protostars?

Free Access

Fig. 1

Density profiles explored in this work. Left panel: 2D hydrogen nucleus number density, n_H = n(H) + 2n(H₂), for the fiducial envelope-only model. Right panel: Same as left panel, but for the fiducial flattened envelope-plus-disk model. In this figure and throughout, log is in base 10.

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.