Open Access

Fig. 1.

image

Download original image

Representative evolution of two 5 M donor stars, one that will experience a DDI, and one that will not. The donor stars fill their Roche lobes at the same moment in their detached evolution (at a size of 15 R), but lose mass in different binary configurations. The DDI system, shown in red, contains an initially 1 M companion star, whilst the stable mass transfer system, shown in blue, starts with an initially 1.5 M companion. Points of interest are labelled with letters, which are explained in the text and Table 1. In the lower left panel, the dotted line shows the mass transfer rate based on the Kelvin-Helmholtz thermal timescale at point A.

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.