Angular momentum relaxation in models of rotating early-type stars

Open Access

Fig. 9.

Prandtl number profiles for a 5 M_⊙ model. The blue line shows the ESTER model with a constant kinematic viscosity of ν = 10⁷ cm²/s. The orange line represents the Prandtl number profile in the envelope based on the polytropic model described in Sect. 4.1.1. For comparison, the radiative Prandtl number, $P_{rad}$ ${\cal {{P}}}_{\mathrm {rad}}$ is also shown (see Eq. (35)).

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.