SMA observations of polarized dust emission in solar-type Class 0 protostars: Magnetic field properties at envelope scales

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Table 6.

Misalignment between the outflow angles χ_o and the mean magnetic field orientation χ_{B₁₀₀₀} in the central 1000 au.

Name	χ_o^a (°)	χ_{B₁₀₀₀} (°)	\| χ_o–χ_{B₁₀₀₀}\|
B335	90	55±3	35
SVS13-A	148	140±3	8
SVS13-B	160	19±6	39
HH797	150	113±2	37
L1448C	161	–	–
L1448N-B	105	23±5	82
L1448-2A	138	–	–
IRAS03282	120	–	–
NGC 1333 IRAS4A	170	57±13	67
NGC 1333 IRAS4B	0	58±49	58
IRAS16293-A	145	163±15	18
IRAS16293-B	130	114±17	16
L1157	146	146±4	0
CB230	172	86±3	86

Notes.

^(a)

Position angles are provided east of north.

References. Bachiller et al. (1998), Bachiller et al. (2001), Choi (2001), Hull et al. (2013), Hull et al. (2014), Rodríguez et al. (1997), Tafalla et al. (2006), Rao et al. (2009), Santangelo et al. (2015), and Yen et al. (2015).

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