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. 2015 Aug 25;7(2):174–186. doi: 10.1080/21505594.2015.1076614

Figure 3.

Figure 3.

Classification of the system trajectories. (A) Homoclinic orbit of the saddle point H (star) when the spiral point L (dot) is stable. (B) The unstable manifold of the saddle point H (star) when the spiral point L (dot) is unstable.