Free Access

Fig. C.1

image

Vertically averaged H2O ice abundance (top), HDO/H2O ice column density ratio (middle), and the ice column density ratio of D2O/HDO to HDO/H2O (bottom) in a disk model around a typical T Tauri star after 1 Myr evolution. The data are taken from Furuya et al. (2013) and Furuya & Aikawa (2014). In regions between the dashed vertical lines, H2O ice is abundant (~10-4) and the cometary HDO/H2O ice ratio is reproduced. The top label represents the temperature in the disk midplane.

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.