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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