Table 2
Comparison between position angle of magnetic field, CH3OH maser distribution, outflows, and linear polarization angles.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
|---|---|---|---|---|---|---|---|---|---|---|
| Source | Φf (a) | ⟨χ⟩(b) | ⟨ΦB⟩(b) | PAoutflow |  |
ρ (c) | |PAoutflow −⟨ΦB⟩| |  |
 |
Ref. |
| (°) | (°) | (°) | (°) | (°) | (°) | (°) | (°) | |||
| G30.70-0.07 (W43-MM2) | 12 | +61 ± 17 | −45 ± 57(d) | − | −63 ± 7 | −0.65 | − | 56 ± 18(e) | − | – |
| G30.76-0.05 (W43-MM11) | 12 | +20 ± 64 | +20 ± 64(d) | − | −30 ± 48 | −0.41 | − | 50 ± 80 | − | - |
| G31.28+0.06 | 10 | +53 ± 35 | −38 ± 33(d) | −26 ± 15(f,g) | +73 ± 4 | +0.39 | 12 ± 36 | 20 ± 35 | 81 ± 16(e) | (1) |
| G32.03+0.06 | 12 | −86 ± 79 | −64 ± 34(d) | − | +32 ± 7 | +0.91 | − | 62 ± 79(e) | − | – |
| G69.52-0.97 | 6 | −29 ± 5 | −51 ± 69(d) | −69 ± 15(h,g) | +23 ± 7(i) | +0.99 | 18 ± 71 | 52 ± 9 | 88 ± 17(e) | (2) |
| From Paper IV(j) | ||||||||||
| G23.44-0.18 (MM2) | 13 | +23 ± 40 | −67 ± 40 | −40 ± 15 | +30 ± 26 | +0.69 | 27 ± 43 | 13 ± 48 | 70 ± 30 | (3) |
| −24 ± 91 | −0.37 | 47 ± 99 | 16 ± 92 | |||||||
| G25.83-0.18 | 11 | +23 ± 7 | −67 ± 7 | +10 ± 15 | +51 ± 7 | +0.69 | 77 ± 17 | 28 ± 10 | 41 ± 17 | (3) |
| G25.71-0.04 | 23 | −51 ± 77 | −80 ± 43 | −90 ± 15 | −71 ± 9 | −0.41 | 10 ± 46 | 20 ± 78 | 18 ± 18 | (3) |
| G28.31-0.39 | 24 | +40 ± 44 | −50 ± 44 | −52 ± 15 | +85 ± 22 | +0.07 | 2 ± 47 | 45 ± 49 | 84 ± 27 | (3) |
| G28.83-0.25 | 10 | −45 ± 34 | +58 ± 59 | −40 ± 15 | −41 ± 10 | -0.83 | 82 ± 61 | 4 ± 35 | 1 ± 18 | (3) |
| G29.96-0.02 | 12 | +62 ± 17 | −29 ± 17 | −38 ± 15 | +80 ± 3 | 0.51 | 9 ± 23 | 18 ± 17 | 62 ± 16 | (3) |
| G43.80-0.13 | 14 | −81 ± 5 | +9 ± 5 | +38 ± 15 | −48 ± 5 | -0.94 | 29 ± 16 | 33 ± 7 | 86 ± 16 | (3) |
| IRAS 20126+4104 | 4 | −70 ± 16 | +20 ± 16 | −65 ± 5 | +87 ± 4 | +0.12 | 85 ± 17 | 23 ± 17 | 28 ± 6 | (3) |
| G24.78+0.08-A2 | 17 | −53 ± 2 | +37 ± 2 | −40 ± 15 | −26 ± 19 | −0.77 | 77 ± 15 | 79 ± 19 | 66 ± 24 | (3) |
| G25.65+1.05 | 7 | −80 ± 8 | −23 ± 51 | −15 ± 15 | −49 ± 7 | −0.87 | 8 ± 53 | 31 ± 11 | 64 ± 17 | (3) |
| G29.86-0.04 | 17 | +46 ± 41 | +82 ± 56 | +6 ± 15 | +8 ± 7 | +0.73 | 76 ± 58 | 38 ± 42 | 14 ± 17 | (3) |
| G35.03+0.35 | 8 | −64 ± 5 | +26 ± 5 | +27 ± 15 | −26 ± 19 | −0.77 | 1 ± 16 | 38 ± 20 | 53 ± 24 | (3) |
| G37.43+1.51 | 4 | +90 ± 3 | +90 ± 3 | −4 ± 15 | −64 ± 5 | −0.87 | 86 ± 15 | 26 ± 6 | 60 ± 16 | (3) |
| G174.20-0.08 | 4 | − | − | −40 ± 15 | −63 ± 16 | −0.45 | − | − | 23 ± 22 | (3) |
| G213.70-12.6-IRS3 | 2 | +20 ± 5 | −70 ± 5 | +53 ± 15 | +63 ± 2 | +0.95 | 57 ± 16 | 43 ± 5 | 10 ± 15 | (3) |
| Cepheus A | 2 | −57 ± 28 | +30 ± 19 | +40 ± 4 | −79 ± 9 | −0.34 | 10 ± 19 | 22 ± 29 | 61 ± 10 | (3) |
| W75N-group A | 3 | −13 ± 9 | +77 ± 9 | +66 ± 15 | +43 ± 10 | +0.96 | 11 ± 18 | 56 ± 14 | 23 ± 18 | (3) |
| NGC7538-IRS1 | 6 | −30 ± 69 | +67 ± 70 | −40 ± 10 | +84 ± 7 | +0.15 | 73 ± 71 | 66 ± 69 | 56 ± 12 | (3) |
| W3(OH)-group II | 4 | +21 ± 45 | −47 ± 44 | − | −59 ± 6 | −0.84 | − | 80 ± 45 | − | (3) |
| W51-e2 | 12 | + 33 ± 16 | − 60 ± 21 | − 50 ± 20 | +57 ± 8 | +0.70 | 10 ± 29 | 24 ± 18 | 73 ± 22 | (3) |
| IRAS18556+0138 | 5 | − 2 ± 11 | + 88 ± 11 | + 58 ± 23 | −40 ± 2 | −0.99 | 30 ± 26 | 42 ± 11 | 82 ± 23 | (3) |
| W48 | 7 | + 23 ± 7 | − 67 ± 7 | − | +55 ± 10 | +0.70 | − | 78 ± 12 | − | (3) |
| IRAS06058+2138-NIRS1 | 4 | + 49 ± 47 | − 49 ± 52 | − 50 ± 15 | +78 ± 7 | +0.64 | 1 ± 54 | 29 ± 48 | 52 ± 17 | (3) |
| IRAS22272+6358A | 2 | − 80 ± 15 | + 9 ± 15 | − 40 ± 15 | −35 ± 11 | −0.87 | 49 ± 21 | 45 ± 19 | 5 ± 19 | (3) |
| S255-IR | 4 | + 36 ± 12 | − 54 ± 12 | + 75 ± 15 | −63 ± 49 | −0.11 | 51 ± 19 | 81 ± 51 | 42 ± 51 | (3) |
| S231 | 4 | + 28 ± 49 | − 62 ± 49 | − 47 ± 5 | +28 ± 8 | +0.97 | 15 ± 49 | 0 ± 50 | 75 ± 9 | (3) |
| G291.27-0.70 | 7 | − 32 ± 5 | + 52 ± 5 | − | −77 ± 14 | − | − | 45 ± 15 | − | (3) |
| G305.21+0.21 | 9 | − 51 ± 14 | 28 ± 14 | − | +48 ± 23 | − | − | 81 ± 27 | − | (3) |
| G309.92+0.47 | 12 | + 2 ± 56 | − 75 ± 56 | − | +35 ± 5 | − | − | 33 ± 56 | − | (3) |
| G316.64-0.08 | 3 | − 67 ± 36 | + 21 ± 36 | − | +34 ± 29 | − | − | 79 ± 46 | − | (3) |
| G335.79+0.17 | 8 | + 44 ± 28 | − 41 ± 28 | − | −69 ± 25 | − | − | 67 ± 38 | − | (3) |
| G339.88-1.26 | 7 | + 77 ± 24 | − 12 ± 24 | − | −60 ± 17 | − | − | 43 ± 29 | − | (3) |
| G345.01+1.79 | 5 | + 5 ± 39 | − 86 ± 39 | − | +74 ± 4 | − | − | 69 ± 39 | − | (3) |
| NGC6334F (central) | 5 | + 77 ± 20 | − 13 ± 20 | + 30 ± 15 | −41 ± 16 | − | 43 ± 25 | 62 ± 26 | 71 ± 41 | (3) |
| NGC6334F (NW) | 5 | − 71 ± 20 | + 19 ± 20 | + 30 ± 15 | −80 ± 38 | − | 11 ± 25 | 9 ± 43 | 70 ± 41 | (3) |
Notes. (a)Foreground Faraday rotation. It was estimated by using Eq. (3) of Paper I. (b)Because of the high uncertainties of the estimated Φf, the angles are not corrected for Φf. (c) Pearson product-moment correlation coefficient −1 ≤ ρ ≤ +1; ρ = + 1 (ρ = − 1) is total positive (negative) correlation, ρ = 0 is no correlation. (d)Before averaging, we use the criterion described in Sect. 3 to estimate the orientation of the magnetic field w.r.t the linear polarization vectors. (e)The differences between the angles are evaluated taking into account that PA ≡ PA ± 180°, ⟨χ⟩ ≡ ⟨χ⟩± 180°, and ⟨ΦB ⟩ ≡⟨ΦB⟩± 180°. (f)Redshifted lobe of the outflow. (g)We consider an arbitrary conservativeerror of 15°. (h)We consider the CO outflow. (i)We consider clusters I and II. (j)Here we omit all the notes that are already indicated in Table 4 of Paper IV.
References. (1) Yang et al. (2018); (2) Kumar et al. (2004); (3) Paper IV and references therein.
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