Fig. 2.
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Accretion rate history of the ten massive PopIII models used in this work. The data for each star are taken from Regan et al. (2020a). The initial accretion rate is similar for each model; however, as the dynamical interaction between the stars and surrounding gas becomes dominant, the stars begin to migrate outwards and away from matter-rich zones and consequently the accretion rate decreases.
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