Glitches in solar-like oscillating F-type stars - Theoretical signature of the base of the convective envelope on the ratios r010

Open Access

Fig. 1.

r₀₁₀ ratios according to the frequency scaled to ν_max. Left: for the Sun (computed from the BISON frequencies; Broomhall et al. 2009; Hale et al. 2016) and KIC 10162436. Right: for KIC 1435467 and KIC 6679371 (data from Lund et al. 2017a).

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.