Backlighting young stellar objects in the Central Molecular Zone - An ensemble-averaged abundance structure of methanol ices

Open Access

Fig. 9

Column densities of H₂O ice (top) and CH₃OH ice (bottom) as a function of reduced extinction, $A_{K, 0}^{*}$ $Mathematical equation: $\akred$$ . Since $A_{K, 0}^{*}$ $Mathematical equation: $\akred$$ traces the dust column integrated along the line of sight within a YSO envelope, it serves as a proxy for projected distance from the centre of the system, with higher $A_{K, 0}^{*}$ $Mathematical equation: $\akred$$ corresponding to smaller impact parameters.

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.