The interacting double white dwarf population with LISA: Stochastic foreground and resolved sources

Open Access

Fig. 2

Break-up of the contributions to ${\dot{f}}_{GW}$ $\[\dot{f}_{\text{GW}}\]$ from the different terms in Eq. (16) for the system shown in Fig. 1, zoomed in around the moment mass transfer begins. We have combined the donor and accretor contributions into a single term for the mass transfer and for the tidal torque term.

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