Table 1 Open in new tab Column 1 gives...

Run	Ω_O	t_O	t₂₈	M_★	M_D	R_D	F
1	0.6	94.5	114.8	0.53	1.17	250	N
2	0.8	94.5	115.4	0.31	1.39	344	N
3	1.0	96.5	118.4	0.25	1.45	433	N
4	1.2	96.5	119.2	0.23	1.47	567	N
5	1.5	98.5	123.3	0.17	1.53	739	Y
6	1.6	102.4	126.7	0.24	1.46	1091	Y
7	1.8	104.4	130.4	0.16	1.54	952	Y

Run	Ω_O	t_O	t₂₈	M_★	M_D	R_D	F
1	0.6	94.5	114.8	0.53	1.17	250	N
2	0.8	94.5	115.4	0.31	1.39	344	N
3	1.0	96.5	118.4	0.25	1.45	433	N
4	1.2	96.5	119.2	0.23	1.47	567	N
5	1.5	98.5	123.3	0.17	1.53	739	Y
6	1.6	102.4	126.7	0.24	1.46	1091	Y
7	1.8	104.4	130.4	0.16	1.54	952	Y

Table 1

Column 1 gives the ID of the simulation, and Column 2 gives the initial rotational frequency, Ω_O. Column 3 gives the time at which the first protostellar object forms, t_O, and Column 4 gives the time at which 28 per cent of the mass is either in the protostellar disc or in protostars, t₂₈. Column 5 gives the mass of the primary protostar at this juncture, M_★, and Columns 6 and 7 give the mass, M_D, and radius, R_D, of the protostellar disc at the same time. Column 8 indicates whether the disc fragments.

Run	Ω_O	t_O	t₂₈	M_★	M_D	R_D	F
1	0.6	94.5	114.8	0.53	1.17	250	N
2	0.8	94.5	115.4	0.31	1.39	344	N
3	1.0	96.5	118.4	0.25	1.45	433	N
4	1.2	96.5	119.2	0.23	1.47	567	N
5	1.5	98.5	123.3	0.17	1.53	739	Y
6	1.6	102.4	126.7	0.24	1.46	1091	Y
7	1.8	104.4	130.4	0.16	1.54	952	Y

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