Stationary spin map predicted by our analytical model (Eq. (16)) for a CB planet in the gaseous regime (γ₂ ≫ n₂) and in an orbit with α = a₁∕a₂ = 1∕3, as a functionof its eccentricity e₂ and the binary mass ratio m₁∕m₀. The white curve indicates the perfectly synchronous state ⟨Ω₂⟩∕n₂ = 1. The white dots represent the positions of the Kepler CB planets in this diagram where the gaseous component is expected to be large and located close to the binary.