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Table 2

Power law index α of the correlation between and as .

Source name λ No. of pts. Cutoff α
(mm)
Serpens Emb 6 0.87 314 13.3 0.523 ± 0.094

Serpens Emb 8 0.87 206 2.85 0.616 ± 0.114
Serpens Emb 8(N) 0.87 42 5.63 0.648 ± 0.277

BHR71 IRS1 1.3 500 1.50 0.594 ± 0.114
BHR71 IRS2 1.3 197 2.58 0.599 ± 0.129

1.3 835 4.80 0.678 ± 0.070
B335 1.5 114 1.11 0.601 ± 0.223
3.0 288 0.20 0.792 ± 0.197

IRAS 16293A/B 1.3 1241 3.00 0.517 ± 0.073

VLA 1623A/B 1.3 61 7.15 0.639 ± 0.447

L1448 IRS2 1.3 358 0.48 0.675 ± 0.101

OMC3 MMS6 1.3 1323 1.39 0.756 ± 0.062
1.3 873 1.54 0.685 ± 0.073

IRAS4A 1.3 890 2.00 0.828 ± 0.065
0.87 2756 2.50 0.864 ± 0.041

Notes. Results from the correlations presented in Fig. B.3. We list the values of the power law indexes α and associated uncertainties obtained from the linear fits, as well as the wavelength of observations λ, the number of points selected in each case, and the cutoff in Stokes I applied.

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