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Table 3

Polarization and magnetic field parameters.

Source σψ (deg) b(0) (deg) Δv (km s-1) Bposψ) (mG) Bpos(b) (mG) Μ/ΦΒ
IRAS 23151+5912 36 47 2.8 0.27 0.23 1.8
IRAS 23033+5951 28 2.7 0.40 2.9
IRAS 23385+6053 46 54 3.9 0.29 0.27 2.0
W3(H2O) 51 39 4.3 1.53 1.74 3.8
W3IRS4 33 12 3.9 1.10 1.81 2.1
IRAS 21078+5211 39 24 2.9 0.92 1.16 2.9
AFGL2591 50 42 3.3 0.59 0.64 3.9
G75.78+0.34 38 8 4.9 0.97 2.12 2.6
S87 IRS1 35 49 2.2 0.43 0.37 3.1
G084.9505-00.691 3.7
G094.6028-01.797 36 2.1 0.19 2.7
G100.3779-03.578 1.7
G108.7575-00.986 3.3
G138.2957+01.555 24 34 3.0 0.62 0.52 2.1
G139.9091+00.197 1.8
S106 37 47 0.9 0.26 0.24 7.1
CepAHW2 36 16 4.0 3.02 4.45 2.1
NGC 7538IRS9 44 3.6 0.58 2.3
NGC 7538IRS1 9 8 3.8 3.12 3.23 2.3
NGC 7538S 44 47 5.0 1.47 1.43 3.1

Notes. σψ and b(0) are the angle dispersions measured directly from the data and via the structure function analysis (Houde et al. 2009). Βpos(σψ) and Bpos(b) are the corresponding magnetic field strength estimates. Δv is measured from the C18O(2–1) IRAM 30 m data with an 11″ beam. ΜΒ is the mass-to-flux ratio.

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