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Table 4
H2 emission line flux ratios for Haro 11B.
| λ | Line | Observationsa | Modelb | |
|
|
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| μm | Fluor. | Collis. | ||
|
|
||||
| 1.162 | H2 2–1 S(1) | 0.2 | 0.4 | 0.0 |
| 1.185 | H2 3–1 S(3) | 0.2 | 0.4c | ... |
| 1.188 | H2 2–0 S(0)+[Fe ii] | 0.9 | 0.2c | ... |
| 1.207 | H2 3–1 S(2) | 0.1 | 0.2 | 0.0 |
| 1.233 | H2 3–1 S(1) | 0.6 | 0.5 | 0.0 |
| 1.238 | H2 2–0 Q(1)+Fe ii? | 0.2 | 0.4 | 0.0 |
| 1.601 | H2 6–4 Q(1) | 0.1 | 0.4 | 0.0 |
| 1.957 | H2 1–0 S(3) | 0.5 | 0.7c | ... |
| 2.034 | H2 1–0 S(2) | 0.3 | 0.5 | 0.3 |
| 2.073 | H2 2–1 S(3) | 0.3 | 0.2 | 0.0 |
| 2.122 | H2 1–0 S(1) | 1.0 | 1.0 | 1.0 |
| 2.223 | H2 1–0 S(0) | 0.2 | 0.6 | 0.3 |
| 2.248 | H2 2–1 S(1) | 0.2 | 0.5 | 0.0 |
Notes.
(b)
Model values by Black & Dishoeck (1987). We adopt their model 1 for fluorescent lines and model S1 for collisionally excited lines.
(c)
Flux ratios are from model 14 by Black & Dishoeck (1987), because these lines are not present in model 1.
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