Fig. 8

Polarisation maps for a collapsing magnetised dense core (face-on view) obtained with the RAMSES code (rmodel = 6.3 × 102 AU). Labels refer to different times of the collapse: t1 = 1.76 × 104 yr, t2 = 1.86 × 104 yr, t3 = 1.94 × 104 yr, and t4 = 2.96 × 104 yr. White contours show 30, 50, 70, and 90 per cent of the 850-μm dust emission (Stokes I) peak and the scale bar to the right gives Ip in Jy/( beam). See Fig. 1 for further information.
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