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Table 2
Statistical results of the integrated hyperfine intensity anomalies (HIAs) of the inner satellite lines (ISLs) and outer satellite lines (OSLs) as function of para-ammonia column density, kinetic temperature, velocity dispersion, the turbulent part of the velocity dispersion, and the total opacity of NH3 (1,1).
| Parameters | Inner satellite lines (ISLs) | Outer satellite lines (OSLs) | |||||
|---|---|---|---|---|---|---|---|
| Slope(a) | Intercept(b) | r(c) | Slope(a) | Intercept(b) | r(c) | ||
| N(para-NH3) (cm−2) | −0.002 | 0.958 | −0.029 | 0.006 | 1.564 | −0.027 | |
| TK (K) | −0.008 | 1.088 | −0.350 | −0.003 | 1.541 | −0.050 | |
| σV (km s−1) | −0.211 | 0.997 | −0.263 | −0.316 | 1.588 | −0.140 | |
| σNT (km s−1) | −0.182 | 0.985 | −0.224 | −0.488 | 1.633 | −0.215 | |
| τ0 | −0.015 | 0.934 | −0.043 | −0.218 | 1.353 | 0.225 | |
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