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Table 4
H2 rotational and ro-vibrational fluxes.
| Transition | λ | Aλ/AKa | Fluxes (10-15 erg cm-2 s-1) | ||||||||
|
|
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| ( μm) | NGC 34 | IRASF 05189–2524 | UGC 05101 | NGC 5135 | NGC 7130 | NGC 7469 | |||||
|
|
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| H2 0–0 S(0) | 28.23 | 0.42 | 32.2 ± 8.0 | <136 | 12.4 ± 4.1 | 18.0 ± 2.9 | 21.9 ± 2.9 | <69 | |||
| H2 0–0 S(1) | 17.04 | 0.64 | 150 ± 12 | 25.2 ± 3.6 | 47.0 ± 7.0 | 220 ± 11 | 116.1 ± 9.8 | 182.0 ± 9.5 | |||
| H2 0–0 S(2) | 12.28 | 0.58 | 61.7 ± 6.1 | 13.3 ± 2.5 | 22.7 ± 2.8 | 88 ± 15 | 37.7 ± 4.4 | 91.7 ± 9.2 | |||
| H2 0–0 S(3) | 9.67 | 0.99 | 194.3 ± 8.7 | 26.3 ± 3.5 | 20.4 ± 2.3 | 233.8 ± 6.1 | 109 ± 11 | 228.5 ± 8.2 | |||
| H2 0–0 S(5) | 6.91 | 0.38 | 87 ± 21 | <100 | 37.6 ± 3.4 | 66.4 ± 10.0 | 67 ± 10 | 91 ± 10 | |||
| H2 1–0 S(0) | 2.22 | 0.95 | 3.1 ± 0.2 | <1.3 | ··· | 6.4 ± 0.2 | 4.3 ± 0.1 | 1.5 ± 0.2 | |||
| H2 1–0 S(1) | 2.12 | 1.02 | 12.4 ± 1.0 | 5.0 ± 0.4 | ··· | 22.2 ± 1.2 | 14.5 ± 0.6 | 5.3 ± 0.5 | |||
| H2 1–0 S(2) | 2.03 | 1.09 | <7.0 | 2.0 ± 0.2 | ··· | 8.9 ± 0.4 | 5.6 ± 0.2 | 1.4 ± 0.2 | |||
| H2 1–0 S(3) | 1.96 | 1.16 | 14.9 ± 0.5 | 6.9 ± 0.4 | ··· | 22.4 ± 0.7 | 15.8 ± 0.6 | 5.3 ± 0.2 | |||
| H2 2–1 S(1) | 2.25 | 0.93 | 1.7 ± 0.2 | <1.3 | ··· | 3.2 ± 0.2 | 1.7 ± 0.1 | <0.9 | |||
| H2 2–1 S(2) | 2.15 | 0.99 | <1.9 | <0.9 | ··· | <1.6 | <1.2 | <0.8 | |||
| H2 2–1 S(3) | 2.07 | 1.06 | <2.0 | <1.2 | ··· | 2.7 ± 0.4 | 1.2 ± 0.2 | <0.8 | |||
| H2 2–1 S(4) | 2.00 | 1.11 | <2.8 | <1.1 | ··· | <3.2 | <1.7 | <1.5 | |||
Notes. Line fluxes and 1σ statistical uncertainties. For non detections, we list the 3σ upper limits. They are observed fluxes not corrected for extinction.
(a)
Interpolated from the Chiar & Tielens (2006) local interstellar medium extinction law.
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