Corner plot showing the results of the Bayesian linear regression performed for the mass-loss rates ( Ṁ) in the CNO grid. As observed, the correlations remain low, except for the same parameters previously mentioned. However, the dispersion continues to follow the decreasing trend, maintaining a high R². This indicates the model performs well in describing the results obtained with our procedure, suggesting it is effective in capturing the relationships between stellar parameters and mass-loss rates.