Fig. 12
Histograms of distance to θ1 Ori C as a function of accretion type. The histogram shows no indication that binaries of any type are more likely at any distance. The vertical dashed line shows the radius (460′′; Reipurth et al. 2007) inside which the ratio of wide binaries (0
5–15) to close binaries (015–05) drops considerably, probably owing to dynamical interaction.
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.