Top left: Companion frequency for a primary mass of 20 M_⊙ at different orbital periods. The blue line represents the companion frequency from Moe & Di Stefano (2017) for a 20 M_⊙ primary, while the other colors show extrapolated companion frequencies for different minimum mass ratios (q_min). Top right: Initial orbital distribution of isolated binaries with a q_min = 0.001. Bottom panels: Initial inner and outer orbital distributions of triple systems with q_min = 0.001.