Fig. 3

Properties of the He layer burning on the surface of WD in the plane of WD mass and accretion rate, in which the super-Eddington wind is triggered when Lprime = LEdd. The red solid line shows the Eddington accretion rate ṀEdd, whereas the green solid line presents the minimum accretion rate Ṁst for stable He layer burning. For comparison, we also present the boundaries of (black dashed line) by setting Lnuc = LEdd and ṀRG (blue dotted line).
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