Open Access

Table F.2

Same as Table F.1 for the distribution of apparent specific angular momentum |japp| along the equatorial axis.

Source Radial range Power law fit Broken power law fit


βapp χ2 rapp,break χ2
(au)−(au) (au)
L1448-2A(⋆⋆) 60−4000 0.3 ± 0.1 1.3 0.1 ± 0.1 1380 ± 400 1.6 ± 0.5 0.6
L1448-NB 150−8200 0.02 ± 0.04 2.3
L1448-C 100−4000 0.69 ± 0.03 5.5 −0.1 ± 0.1 790 ± 100 1.6 ± 0.1 2.0
IRAS2A(⋆⋆) 85−8200 1.4 ± 0.1 6.2 0.3 ± 0.1 2180 ± 110 28.4 ± 22.2 2.5
SVS13-B 110−1900 1.0 ± 0.1 1.5 0.1 ± 0.3 640 ± 190 2.2 ± 0.5 0.2
IRAS4A 250−1600 1.9 ± 0.1 0.9 −0.3 ± 0.7 470 ± 60 2.1 ± 0.2 0.4
IRAS4B 175−3100 1.5 ± 0.1 4.0
IRAM04191(⋆⋆) 55−9700 0.8 ± 0.1 0.5
L1521F 1500−4200 1.2 ± 0.6 0.1
L1527(⋆⋆) 45−7800 −0.12 ± 0.03 1.8 −0.14 ± 0.03 1320 ± 260 1.3 ± 0.2 1.6
L1157(⋆⋆) 85−9800 0.8 ± 0.1 0.4
GF9-2(⋆⋆) 75−5600 0.5 ± 0.1 2.3 0.3 ± 0.1 980 ± 370 1.2 ± 0.3 1.0

Median profile 45−9800 0.9 ± 0.1 0.3 ± 0.3 1570 ± 300 1.6 ± 0.2

Notes. Here, we consider all the velocity gradients observed at all envelope scales, including the reversed gradients and the shifted ones at scales of r ≳1000 au (see Fig. 19 and Sect. 5.4) which were excluded in the construction of the PVrot diagrams in Fig. 16, and in Table F.1 for our analysis of rotational motions. (⋆⋆) Sources with a negative apparent specific angular momentum along the equatorial axis in the outer envelope scales of r > 1600 au (see Sect. 5.4.1).

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