Fig. 18.
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Comparison of the mass growth rate (top panel) and the growth rate due to stellar collisions (bottom panel) as a function of the mass of the MMO for temperatures of 8000 K, 3000 K, and 500 K with the theoretical accretion rates of Bondi-Hoyle (red line) and accretion regulated by self-gravity (orange line) from Schleicher et al. (2023).
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