Free Access

Table 1.

Models used for comparison.

Name Code Base model L (L) Teff (K) Notes
CO5BOLD mean CO5BOLD st28gm06n26 6955 2737 Mean structure of a 3D model.
CO5BOLD x-dir CO5BOLD st28gm06n26 6955 2737 Local structure of a 3D model.
DARWIN u2 DARWIN l70t27 7000 2700 Δup = 2 (from Eqs. (1) and (2))
DARWIN u4 DARWIN l70t27 7000 2700 Δup = 4 (from Eqs. (1) and (2))

Notes. Two ways are used to extract radial velocities and luminosity from a 3D model, either by considering the mean behaviour of the structure or the local behaviour (see Sect. 3 for more detailed explanation). This is compared to two DARWIN models, with the same stellar parameters but different inner boundary conditions.

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.