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Table 5

Parameters derived from N2H+(3−2) data.

N(N2H+) x(N2H+) N(NH3)/N(N2H+) σ NT f turb
Source [1013 cm-2] [10-10] [km s-1]

IRAS 05399-0121 2.0 ± 0.7 4.3 ± 1.8 16 ± 7 0.28 ± 0.03 1.3 ± 0.2
SMM 1 1.9 ± 1.1 5.9 ± 3.4 32 ± 18 0.25 ± 0.04 1.2 ± 0.2
SMM 3 0.6 ± 0.1 0.8 ± 0.2 99 ± 25 0.30 ± 0.01 1.5 ± 0.1
IRAS 05405-0117 1.0 ± 0.2a 5.5 ± 1.5 100 ± 28 0.28 ± 0.03 1.4 ± 0.1
SMM 4b
SMM 4 (2nd v-comp.) 0.2 ± 0.2 0.8 ± 0.6 288 ± 225 0.18 ± 0.11 0.9 ± 0.6
SMM 5 0.1 ± 0.1 0.7 ± 0.4 562 ± 279 0.19 ± 0.06 0.9 ± 0.3
0.2 ± 0.03c 1.2 ± 0.2c 275 ± 54c
SMM 6 0.6 ± 0.2 2.1 ± 0.6 194 ± 80 0.24 ± 0.04 1.2 ± 0.2
Ori B9 N 0.02 ± 0.03 0.2 ± 0.3 916 ± 1345d 0.07 ± 0.18c 0.3 ± 0.8
0.1 ± 0.2c,d 0.8 ± 0.1c 280 ± 190c
Ori B9 N (2nd v-comp.) 0.1 ± 0.04 0.6 ± 0.5 250 ± 90 0.17 ± 0.10 0.8 ± 0.5
0.1 ± 0.05c 1.1 ± 0.4c 250 ± 154c
SMM 7 0.1 ± 0.1 0.3 ± 0.2 718 ± 553 0.28 ± 0.10 1.5 ± 0.5
0.3 ± 0.1c 0.7 ± 0.3c 267 ± 91c

Notes.

(a)

In Paper I, we derived the value N(N2H+) ≈ 0.91 ± 0.01 × 1013 cm-2 from observations of N2H+(1−0) emission, which is in good agreement with the present value.

(b)

The principal velocity component was not detected.

(c)

Calculated by using the optically thin approximation.

(d)

The associated error is larger than the value.

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