Back to the Abstract

	1 Introduction
	2 Observations of cores
	3 Observations of stars and binary systems
	4 Outline of model
	5 Dimensionless simulations
	6 Convolving with the core-mass spectrum
	7 Convolving with the distribution of core rotation rates
	8 Conclusions
	Appendix A: Skewing the log-normal distribution of stellar masses
	References

	List of tables
	List of figures