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Table 3.

Comparison of observable quantities from the star formation models with our observations.

Parameter Core accretion Competitive accretion Collisions This work
CF CF ∝ mass CF ∝ mass CF ∝ mass
IMF Top heavy Top heavy Strong deviation from Salpeter IMF Salpeter IMF
m2 and m1 Correlated Uncorrelated or slightly correlated
r and M Correlated r ∝ M−2 Uncorrelated
q and r anticorrelated Most q ≤ 0.5 uncorrelated

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