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Table 4

Position angles of the outflow and magnetic field and velocity gradients characteristics.

Name Outflow Bmean Line used Velocity gradients


PA(a) Ref. PA Gradient PA Ref.
(°) (°) (km s−1 pc−1) (°)
Per B1-bS 120 [1] 26 ± 7 N2 D+ 23 ± 3 −8 ± 8 [26] & T. w.
Per B1c 125 [2] 99 ± 39 N2 H+ 7.5 50 [2] & T. w.
B335 90 [3] 55 ± 3 N2 H+ ~1.0 [24]
BHR7-MMS 174 [4] 87 ± 19 N2 D+ 14 ± 1.0 −36 ± 6 [4] & T. w.
CB230 172 [5] 85 ± 4 N2 H+ 3 ± 0.1 98 ± 1.3 [21]
HH25-MMS [6] 74 ± 17
HH211-mm 116 [7] 174 ± 5 N2 H+ 7 ± 0.03 26 ± 0.3 [21,23]
HH212 23 [8] 51 ± 4 NH3 4.5 113 [22]
HH797 150 [9] 110 ± 7
IRAS 03282 120 [10] 43 ± 6 N2 H+ 9 ± 0.01 114 ± 0.01 [21]
IRAS 16293-A 75 & 145 [11] 173 ± 40 CN 25 [25]
L1157 146 [12] 149 ± 4 N2 H+ 0.8 ± 0.4 113 ± 65 [20]
L1448C 162 [13] 95 ± 4 N2 H+ 13 ± 1 –179 ± 1.0 [20]
L1448N-B 105 [14] 23 ± 4 N2 H+ 13 ± 1 100 ± 1 [20]
L1448-2A 134 [5] 139 ± 9 (b) N2 H+ 2 ± 1 –177 ± 21 [20]
L483 105 [15] 8 ± 11 N2 H+ 9 ± 0.03 45 ± 0.2 [21]
NGC 1333 IRAS4A 20 [16] 55 ± 13 N2 H+ 7 ± 1 37 ± 2 [20]
NGC 1333 IRAS4B 0 [17] 51 ± 19 N2 H+ 3 ± 1 −71 ± 14 [20]
Serp SMM18 8 [18] 84 ± 16 N2 H+ 12 ± 0.01 69 ± 0.04 T. w.
SVS13-B 160 [19] 18 ± 5 N2 H+ 5 ± 1 16 ± 4 [20]

Notes. (a) Position angles in the table are provided east of north. (b)Taken from Hull et al. (2013).

References. T. w. refers to “this work”, [1] Gerin et al. (2015), [2] Matthews et al. (2008), [3] Hirano et al. (1988), [4] Tobin et al. (2018), [5] Hull et al. (2013), [6] Dunham et al. (2014), [7] Gueth & Guilloteau (1999), [8] Lee et al. (2017), [9] Tafalla et al. (2006), [10] Hatchell et al. (2007), [11] Rao et al. (2009), [12] Bachiller et al. (2001), [13] Dutrey et al. (1997), [14] Kwon et al. (2006), [15] Oya et al. (2018), [16] Choi et al. (2006), [17] Choi (2001), [18] Maury et al. (2019), [19] Bachiller et al. (1998), [20] Gaudel et al. (2020), [21] Tobin et al. (2011), [22] Wiseman et al. (2001), [23] Tanner & Arce (2011), [24] Saito et al. (1999), [25] Antonio Hernández-Gòmez’s (PhD thesis, priv. comm.) [26] Huang & Hirano (2013).

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