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This article is an erratum for:

Volume 570, October 2014
Article Number C4
Number of page(s) 2
Section Stellar structure and evolution
Published online 03 November 2014

An error occurred during the production process. An incorrect Fig. 12 was published. The correct Fig. 12 is published on the following page.

thumbnail Fig. 12

Five best fit models (from top to bottom, following the order in Table 6) using frequencies from MESA/GYRE. Upper panels: observed peaks (red circles, the error bars are smaller than the symbol size) versus the theoretical frequencies of the = 1 gravity modes (blue crosses, with the corresponding n value printed above). Lower panels: individual spacing values between the members of the observed period series (red filled circles) and the δp(p) function from the model (blue solid line).

© ESO, 2014

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