Open Access

Table 1.

Computed critical densities (cm−3) for fine structure IR lines from PYNEB, for different electronic temperatures.

Emission line Te = 5000 K Te = 10 000 K Te = 15 000 K Te = 20 000 K Te = 25 000 K Te = 30 000 K
[S IV]λ10.5 μm 4.0 × 104 5.6 × 104 6.9 × 104 7.9 × 104 8.8 × 104 9.6 × 104
[Ne II]λ12.8 μm 4.6 × 105 6.3 × 105 7.4 × 105 8.4 × 105 9.2 × 105 1.0 × 106
[Ne V]λ14.3 μm 1.8 × 104 3.2 × 104 4.7 × 104 6.3 × 104 7.8 × 104 9.3 × 104
[Ne III]λ15.6 μm 1.5 × 105 2.1 × 105 2.5 × 105 2.8 × 105 3.0 × 105 2.9 × 105
[S III]λ18 μm 8173 1.2 × 104 1.5 × 104 1.7 × 104 1.8 × 104 2.0 × 104
[Ne V]λ24 μm 3579 5952 8426 1.1 × 104 1.3 × 104 1.6 × 104
[O IV]λ26 μm 8387 9905 1.2 × 104 1.3 × 104 1.4 × 104 1.5 × 104
[S III]λ33 μm 980 1417 1801 2140 2425 2686
[O III]λ52 μm 2753 3530 3879 4082 4233 4418
[N III]λ57 μm 1180 1519 1723 1859 1938 1971
[O III]λ88 μm 388 501 569 620 662 704
[N II]λ122 μm 198 238 256 267 276 283
[N II]λ205 μm 30 38 44 47 51 54

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