Fig. 22.
Download original image
Stellar radius versus orbital period for DPVs (left). The arrow indicates the position of V 4142 Sgr and the solid line the best second-order polinomial fit for the donor star data. Right: temperatures for the hot and cool stellar components of DPVs. The arrow indicate the position of V 4142 Sgr and the solid line is the best 2nd order polinomial fit to the data.
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.