Open Access

Fig. 3


Illustration of the ejecta regions (in velocity space) at the origin of the optical flux for model DDC15 with Mst = 0.18 M at 200 d. The top panel shows a gray linear scale of the (emergent) luminosity δLλ,V while the bottom panel shows the contributions (ordinate in logarithmic space) for the full ejecta and those fromthe stripped material (blue) or the metal-rich ejecta (red). As is evident from these plots, the predominant emerging feature due to stripped material of the companion star at optical wavelengths is Hα.

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.