A robust model for the origin of optical quasi-periodic variability in supersoft X-ray sources

Open Access

Fig. 5.

Similar to Fig. 4, but for the model with an initial WD mass of M_WD = 1.2 M_⊙ and different accretion rates at point B (see the panel c of Fig. 3). Panelsa–d show the cases with , , , and , respectively, and the exact values of are given in each panel.

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