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Table 2
Best-fit parameters for the proton distributions (see Eq. (1)) in Gould Belt clouds.
| Name | N0,1044 V-1 | i 1 | rbr, GV | i 2 | s |
|
|
|||||
| R CrA |
|
|
|
|
16.06 (>1.03) |
| Rho Oph |
|
|
|
|
20.61 (>0.84) |
| Perseus |
|
|
|
|
9.55 (>0.88) |
| Chameleon |
|
|
|
|
11.19 (>0.88) |
| Cepheus |
|
|
|
|
71.02 (>1.02) |
| Taurus |
|
|
|
|
56.46 (>1.05) |
| Orion A |
|
|
|
|
230.94 (>1.00) |
| Orion B |
|
|
|
|
17.90 (>1.09) |
| Mon R2 |
|
|
|
|
89.20 (>0.80) |
|
|
|||||
| All |
|
|
|
|
62.52 (>1.50) |
Notes. For the break strength, the best-fit value and 95% lower limits are given. Note that the normalisations N0 are scaled to the distance to the cloud D = 1 kpc, and the cloud density is n = 1 cm-3.
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