A transition from mixed-fuel to pure-helium thermonuclear bursts in Terzan 5 X–3/Swift J174805.3–244637

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Fig. 7.

Recurrence time versus local mass accretion rate. The dashed line represents the best-fit power-law model for all bursts: $Δ T_{rec} \propto {\dot{m}}^{- 1.31 \pm 0.04}$ $\Delta T_{\mathrm{rec}} \propto \dot{m}^{-1.31 \pm 0.04}$ .

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