High-mass eclipsing binaries: A testbed for models of interior structure and evolution - Accurate fundamental properties and surface chemical composition for V1034 Sco, GL Car, V573 Car, and V346 Cen

Open Access

Fig. 15.

Stochastic low-frequency variability of V346 Cen. Top: part of the (out-of-eclipse) residual light curve of V346 Cen, after fitting the orbital harmonics. Bottom: Lomb–Scargle periodogram, calculated for the out-of-eclipse data points of the residual light curve for sectors 37 and 38.

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.