Table 1: The numbers of different multiple systems produced in the dimensionless simulations.
${\cal N} = 3$ ${\cal N} = 4$ ${\cal N} = 5$ ${\cal N} = 6$

$\sigma_{\log m}=0.2$ S 33 253 39 711 43 873 46 567

B 33 241 22 506 20 207 19 306

T 88 5091 5014 4394

Q 0 1 168 409

mf 0.5001 0.4100 0.3666 0.3411

$\sigma_{\log m}=0.4$ S 33 231 41 883 45 534 48 053

B 33 228 22 073 18 033 16 670

T 104 4657 5764 5389

Q 0 0 277 609

mf 0.5008 0.3896 0.3459 0.3205

$\sigma_{\log m}=0.6$ S 33 161 40 950 41 598 47 707

B 33 155 23 098 16 955 16 378

T 176 4282 5645 5726

Q 0 1 333 589

mf 0.5013 0.4007 0.3554 0.3223

**Table 1:** The numbers of different multiple systems produced in the dimensionless simulations.
		${\cal N} = 3$	${\cal N} = 4$	${\cal N} = 5$	${\cal N} = 6$
$\sigma_{\log m}=0.2$	S	33 253	39 711	43 873	46 567
	B	33 241	22 506	20 207	19 306
	T	88	5091	5014	4394
	Q	0	1	168	409
	mf	0.5001	0.4100	0.3666	0.3411
$\sigma_{\log m}=0.4$	S	33 231	41 883	45 534	48 053
	B	33 228	22 073	18 033	16 670
	T	104	4657	5764	5389
	Q	0	0	277	609
	mf	0.5008	0.3896	0.3459	0.3205
$\sigma_{\log m}=0.6$	S	33 161	40 950	41 598	47 707
	B	33 155	23 098	16 955	16 378
	T	176	4282	5645	5726
	Q	0	1	333	589
	mf	0.5013	0.4007	0.3554	0.3223

Source LaTeX | All tables | In the text

	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