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Table 4

Examined parameters and their behavior in the cases of modified disk and competitive accretion.

Parameter Expectation from SADA Expectation from CA Observed

CSF and M1 correlated correlated correlated
CMF Salpeter IMF; top-heavy for massive primaries Strong deviation from Salpeter IMF for massive primaries Γ ≈  − 0.001
M   and   R correlated anticorrelated i.e. R ~ M2x − 3 anticorrelated (uncertain), x = 1.22
m   and   R no statement anticorrelated anticorrelated (uncertain)
M   and   m no correlation correlated correlated
M2   and   M1 correlated correlated correlated

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