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Table 1.

Varied input parameters and global properties of the simulations.

Case B*/B0 Υ Φopen* Υopen rA⟩/R* acc/0 Υacc Rt/R* τsw/τacc τme/τacc
1 (a) 0.8125 5030 0.296 441 7.98
2 (a) 1.625 25 800 0.230 1360 12.0
3 (a) 3.25 130 000 0.172 3860 17.6
4 (a) 6.5 635 000 0.131 10900 25.6
5 (a) 13 2 960 000 0.0951 26700 33.9

1 (b) 1.625 45 000 0.381 6550 23.4 0.489 3.82 1.82 −0.355 0.486
2 (b) 3.25 139 000 0.267 9890 28.1 0.628 11.9 2.64 −0.416 0.219
3 (b) 6.5 667 000 0.164 18000 37.0 0.861 34.7 4.04 −0.359 0.111
4 (b) 9.75 2 220 000 0.114 28900 44.9 1.20 55.9 4.68 −0.221 −0.0237
5 (b) 13 5 420 000 0.0873 41300 52.5 1.61 74.4 4.92 −0.173 −0.0853

Notes.

(a)

ISW simulations.

(b)

SDI simulations. In our simulations, a negative (positive) torque indicates angular momentum flowing toward (away from) the star (see also Sect. 3.1.1). Consequently, τsw >  0, τacc <  0, and τme ≶ 0 (for the sign of τme in each SDI case, see also Fig. 10).

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