Table 2
Parameters used for calculating the turbulent Bturb and regular magnetic field strengths Breg.
| Region | ν (GHz) | TI (mJy) | PI (mJy) | P (%) | α | i (°) | z (pc) | Bturb (μG) | Breg (μG) | Location |
|
|
||||||||||
| 1 | 8.44 | 488 | 0.125 | 0.026 | –0.60 | 11 | 900 | 140 | 0.8 | centre |
| 2 | 8.44 | 98 | 0.255 | 0.258 | –1.44 | 30 | 250 | 124 | 11.4 | bar |
| 3 | 8.44 | 0.89 | 0.11 | 12.00 | –0.88 | 11 | 900 | 22 | 7.5 | halo |
| 1 | 4.86 | 678 | 0.275 | 0.041 | –0.60 | 11 | 900 | 140 | 1.1 | centre |
| 2 | 4.86 | 144 | 0.224 | 0.155 | –1.44 | 30 | 250 | 113 | 8.4 | bar |
| 3 | 4.86 | 1.43 | 0.133 | 9.28 | –0.88 | 11 | 900 | 22 | 6.5 | halo |
| 4 | 1.54 | 1249 | 0.076 | 0.006 | –0.62 (–0.14) | 11 | 900 | 117 | 0.3 | centre |
| 5 | 1.54 | 89 | 0.049 | 0.056 | –0.84 | 30 | 250 | 67 | 1.3 | bar |
| 6 | 1.54 | 33 | 0.014 | 0.041 | –1.40 | 11 | 900 | 24 | 0.9 | halo |
| 7 | 1.54 | 5.37 | 0.159 | 2.90 | –1.68 | 11 | 900 | 17 | 4.2 | halo |
| 8 | 1.54 | 1.40 | 0.132 | 9.44 | –1.26 | 11 | 900 | 10 | 3.7 | halo |
| 9 | 1.54 | 0.47 | 0.243 | 51.4 | –1.61 | 11 | 900 | 5.8 | 7.5 | halo |
Notes. Regions are numbered as in the images. ν is the average observing frequency, TI, P, and α are the average total intensity, polarised intensity, and spectral indices over the integrated area, FP is the average fractional polarisation calculated from P/TP, i the inclination of the regular magnetic field towards the observer, and z the assumed path length of the emitting medium. The most likely location of the detected structure is given in the last column.
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