Fig. 3
Predicted GW Lib instability strips for models with envelope compositions ranging from solar (upper left figure of upper panel) to a H-less mixture (lower right figure of lower panel). The dotted vertical lines correspond to the effective temperature for each of the 11 pulsating white dwarfs of the GW Lib type listed in Table 6 of Szkody et al. (2010).
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.