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Table 1

Parameters of the simulations described in the text.

Case λ α B,J t M in M M disc
[rad] [kyr] [ M ] [ M ] [ M ]

L 1 5 0 0.824 1
L 2 5 π/2 10.756 1 0.46 0.28
H ~2 no initial rotation 6.000 100 1.24a 0.87a

Notes. Columns: non-dimensional mass-to-flux ratio λ, initial angle between the magnetic field direction and the rotation axis αB,J, time after the formation of the first Larson’s core t (core formed in the centre of the pseudo-disc with n ≳ 1010 cm-3 and r ~ 10–20 AU), initial mass Min, mass of the protostellar core M and of the disc Mdisc.


This value refers to the densest fragment formed.

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