Table 2
Polarised intensities and magnetic field parameters.
Core | Ipeak | Ipol (a) | σψ (b) | σν (c) | ![]() |
b | ![]() |
Bt∕B0 | |||
---|---|---|---|---|---|---|---|---|---|---|---|
(mJy beam−1) | (mJy beam−1) | (°) | (km s−1) | (mG) | (°) | (mG) | |||||
MM3 | 27.6 | 2.79 ± 0.07 | 41.8 ± 0.1 | 2.00 ± 0.01 | 0.33 ± 0.02 | 11.9 ± 0.2 | 3.30 ± 0.07 | 0.2 | |||
MM4 | 321.6 | 1.80 ± 0.06 | 28.0 ± 0.4 | 2.00 ± 0.01 | 1.57 ± 0.02 | 9.4 ± 0.3 | 13.18 ± 0.42 | 0.1 | |||
MM7 | 168.9 | 0.66 ± 0.08 | – | – | – | – | – | – | |||
MM8a | 366.7 | 1.74 ± 0.08 | 30.5 ± 3.8 | 2.35 ± 0.01 | 1.64 ± 0.02 | 8.6 ± 0.4 | 17.10 ± 0.75 | 0.1 | |||
MM8c | 44.6 | 1.25 ± 0.08 | – | – | – | – | – | – | |||
MM9 | 63.4 | 0.91 ± 0.07 | – | – | – | – | – | – | |||
MM11a | 42.8 | 0.54 ± 0.10 | – | – | – | – | – | – |
Notes. (a) Ipol are taken at thepeak of the polarised intensity. In case of MM3 and MM4 the peak is located in MM3a and MM4a, respectively. (b) All the values of σψ are obtained using the classical variance, calculated around the circular mean (Jammalamadaka & SenGupta 2001; Pewsey et al. 2013), over regions covering MM3, MM4, and MM8. (c)All the values ofσν are obtained by Liu et al. 2017, Table 3, using methanol emissions.
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