Non-linear three-mode coupling of gravity modes in rotating slowly pulsating B stars - Stationary solutions and modeling potential

Open Access

Fig. 3.

Empirical probability distributions of |δω / (γ₂ + γ₃)| for the 21 identified (stable and AE -valid) isolated mode triads (blue and dotted) and their AE -valid and stable counterparts (yellow) that do not fulfill the isolation criterion. We choose the bin width in a similar way to what is done in Hogg (2008).

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