A semi-analytic model in python for showing the evolution of the power-law stellar IMF due to Bondi-Hoyle-Lyttleton accretion (as seen in Kuznetsova et al, 2018b)

Probability distribution functions of measured protostellar properties (magnetization, specific angular momentum, accretion behavior, mass, etc) from the Athena simulations in Kuznetsova et al (2020).