Influence of stellar structure, evolution, and rotation on the tidal damping of exoplanetary spin-orbit angles

Free Access

Table 3

Values of the magnetic braking model parameters depending on stellar mass, used to compute the evolutions shown in Fig. 6–9, for all initial rotation rates.

	1 M_⊙	1.2 M_⊙
Ω_sat	10 Ω_⊙	42 Ω_⊙
K_w	1.71 × 10³³ kg m² yr	1.71 × 10³³ kg m² yr

Notes. We use Ω_⊙ = 89.94 yr⁻¹ and Ω_crit = 3.89Ω_⊙.

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.