Signatures of magnetic braking in Class 0 protostars: Exploring the gas kinematics in magnetized models of low-mass star formation

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Volume 687 (July 2024)

A&A, 687 (2024) A63

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Table C.2

Parameters fitted by the broken power law in the synthetic observation radial profiles of Fig. 7. In profiles where the fit placed the inflection point beyond the profile limits, the fit was repeated with a simple power law, and in these cases a single slope is presented.

ID	$j_{vmax}^{obs}$ $j_{{\rm{vmax}}}^{{\rm{obs}}}$			$j_{vGauss}^{obs}$ $j_{{\rm{vGauss}}}^{{\rm{obs}}}$			$j_{vpeak}^{obs}$ $j_{{\rm{vpeak}}}^{{\rm{obs}}}$
	in	out	(au)	in	out	(au)	in	out	(au)

μ3ℳ0;0.06Μ_⊙	0.42 ± 0.01	0.82 ± 0.01	765.56 ±32.8	0.12 ± 0.12	0.86 ± 0.01	198.87 ± 22.8	−0.022 ± 0.096	0.916 ± 0.03	217.497 ± 21.646
μ3ℳ0;0.18Μ_⊙	0.43 ± 0.02	0.74 ± 0.02	1221.63 ± 110.83	1.1 ± 0.06	0.51 ± 0.02	399.31 ± 41.29	0.72 ± 0.02	−1.469 ±0.445	1145.789 ± 34.643
μ3ℳ0;0.30Μ_⊙	0.32 ± 0.01	1.1 ± 0.07	2203.47 ± 92.1	0.47 ± 0.11	0.83 ± 0.07	413.78 ± 156.05	0.226 ± 0.102	0.928 ± 0.107	429.166 ± 93.732

μ3ℳ1;0.06Μ_⊙	0.85 ± 0.01			0.94 ± 0.01			0.406 ± 0.05	1.45 ± 0.032	817.339 ±79.379
μ3ℳ1 ;0.18Μ_⊙	0.53 ± 0.01	0.89 ± 0.01	886.67 ± 36.49	0.59 ± 0.03	0.94 ± 0.02	796.19 ± 91.52	0.58 ± 0.01	1.39 ± 0.04	1733.95 ± 55.74
μ3ℳ1;0.30Μ_⊙	0.46 ± 0.01	0.93 ± 0.02	1329.3 ± 56.9	0.87 ± 0.03			0.86 ± 0.03

μ10ℳ0;0.07Μ_⊙	0.73 ± 0.05	0.39 ± 0.01	246.0 ± 26.56	0.6 ± 0.01	0.77 ± 0.02	1690.28 ± 116.86	0.695 ± 0.03	0.505 ± 0.003	172.417 ± 21.569
μ10ℳ0;0.18Μ_⊙	0.67 ± 0.02	0.19 ± 0.01	580.6 ± 32.97	0.88 ± 0.04	0.27 ± 0.02	578.99 ± 46.83	0.719 ± 0.017	0.133 ± 0.01	651.853 ± 24.742
μ10ℳ0;0.30Μ_⊙	0.57 ± 0.02	−0.2 ± 0.03	1418.48 ±53.66	0.83 ± 0.01	−0.46 ± 0.04	1808.66 ±31.71	0.71 ± 0.012	−0.716 ± 0.043	1833.287 ±32.848

μ10ℳ1;0.06Μ_⊙	0.574 ± 0.003	1.0 ± 0.05	2917.16 ± 74.47	0.73 ± 0.01	−0.004 ± 0.045	2370.75 ± 54.76	0.678 ± 0.003	1.67 ± 0.38	3690.14 ± 67.77
μ10ℳ1;0.18Μ_⊙	0.49 ± 0.01	−0.19 ± 0.86	3724.02 ± 208.8	0.81 ± 0.04	0.38 ± 0.01	331.94 ± 24.95	0.69 ± 0.03	0.43 ± 0.01	291.59 ±34.76

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