Three-dimensional hydrodynamical simulations of red giant stars: semi-global models for interpreting interferometric observations

Free Access

Fig. 1

Open with DEXTER Download original image

Intensity maps in the optical top-hat filter of Fig. 3 for the simulation with log g = 1.6 and [Fe/H ] = −3.0 (Table 1) with μ = 1.00, 0.81, 0.58, and 0.40. The intensities typically ranges from 3 × 10⁴ to 1.2 × 10⁶ erg cm^-2 s^-1 Å^-1.

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.