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Table B.1.
Integrated fluxes of H2 lines in all sources and apertures, corrected for extinction
| Pos. | Integrated flux ×10−18 [W m−2] | |||||||
|---|---|---|---|---|---|---|---|---|
| S(1) | S(2) | S(3) | S(4) | S(5) | S(6) | S(7) | S(8) | |
| GSS30-IRS 1 | ||||||||
| A | – | – | 303.0 ± 73.0 | 50.2 ± 10.1 | 77.1 ± 15.6 | 10.9 ± 6.1 | 65.5 ± 9.0 | – |
| B | – | – | 6.8 ± 1.9 | 4.1 ± 1.3 | 19.5 ± 2.2 | 9.0 ± 1.7 | 15.3 ± 2.1 | – |
| C | 1.4 ± 0.3 | 1.6 ± 0.5 | 2.3 ± 0.6 | 2.4 ± 0.7 | 3.9 ± 0.7 | 2.1 ± 1.4 | 4.5 ± 1.2 | – |
| ISO-Oph 21a | ||||||||
| A | 0.6 ± 0.1 | 0.9 ± 0.1 | – | – | – | – | – | – |
| B | 0.8 ± 0.1 | 1.1 ± 0.1 | – | – | – | – | – | – |
| C | 0.6 ± 0.1 | 1.1 ± 0.1 | – | – | – | – | – | – |
| D | 0.8 ± 0.1 | 1.1 ± 0.1 | – | – | – | – | – | – |
| E | 0.6 ± 0.1 | 1.1 ± 0.1 | – | – | – | – | – | – |
| [GY92] 197 | ||||||||
| A | 1.7 ± 0.1 | 2.4 ± 0.2 | 6.0 ± 0.5 | 1.8 ± 0.2 | 2.8 ± 0.2 | 0.7 ± 0.1 | 1.5 ± 0.2 | 0.3 ± 0.2 |
| B | 0.4 ± 0.1 | 0.6 ± 0.1 | 1.3 ± 0.2 | 0.6 ± 0.1 | 1.3 ± 0.1 | 0.5 ± 0.1 | 0.9 ± 0.2 | 0.2 ± 0.2 |
| C | 0.9 ± 0.1 | 1.3 ± 0.1 | 3.9 ± 0.4 | 1.5 ± 0.2 | 2.1 ± 0.2 | 0.8 ± 0.2 | 1.5 ± 0.2 | 0.5 ± 0.2 |
| D | 1.1 ± 0.1 | 1.9 ± 0.1 | 4.7 ± 0.4 | 1.9 ± 0.2 | 3.2 ± 0.2 | 1.2 ± 0.2 | 2.5 ± 0.3 | 0.8 ± 0.2 |
| E | 1.3 ± 0.3 | 2.4 ± 0.3 | 5.3 ± 0.5 | 1.5 ± 0.2 | 2.3 ± 0.2 | 0.6 ± 0.1 | 1.3 ± 0.2 | – |
| F | 0.4 ± 0.1 | 1.1 ± 0.1 | 1.7 ± 0.5 | 0.6 ± 0.2 | 1.4 ± 0.1 | 0.4 ± 0.1 | 1.0 ± 0.2 | – |
| G | 0.7 ± 0.1 | 1.6 ± 0.2 | 2.7 ± 0.5 | 1.0 ± 0.1 | 1.5 ± 0.2 | 0.4 ± 0.1 | 0.7 ± 0.1 | 0.1 ± 0.2 |
| H | 0.6 ± 0.1 | 1.1 ± 0.1 | 2.7 ± 0.4 | 0.7 ± 0.2 | 1.2 ± 0.1 | 0.2 ± 0.1 | 0.6 ± 0.2 | 0.2 ± 0.2 |
| WL 17 | ||||||||
| A | 0.6 ± 0.2 | 1.7 ± 0.2 | 3.5 ± 0.3 | 1.3 ± 0.1 | 2.3 ± 0.2 | 0.5 ± 0.1 | 1.4 ± 0.2 | 0.4 ± 0.1 |
| B | 0.5 ± 0.1 | 0.8 ± 0.1 | 2.4 ± 0.2 | 0.9 ± 0.1 | 1.8 ± 0.2 | 0.5 ± 0.1 | 1.2 ± 0.2 | 0.5 ± 0.2 |
| C | 0.6 ± 0.1 | 1.2 ± 0.1 | 4.1 ± 0.3 | 1.5 ± 0.1 | 3.1 ± 0.2 | 0.7 ± 0.1 | 2.0 ± 0.2 | 0.5 ± 0.1 |
| D | 0.6 ± 0.2 | 1.2 ± 0.2 | 3.2 ± 0.3 | 1.1 ± 0.1 | 2.6 ± 0.2 | 0.6 ± 0.1 | 1.8 ± 0.2 | 0.2 ± 0.1 |
| E | 0.8 ± 0.2 | 1.9 ± 0.2 | 3.5 ± 0.3 | 1.3 ± 0.1 | 2.1 ± 0.2 | 0.7 ± 0.1 | 1.6 ± 0.2 | 0.5 ± 0.1 |
| F | 0.5 ± 0.1 | 0.7 ± 0.1 | 1.2 ± 0.2 | 0.4 ± 0.1 | 0.8 ± 0.1 | 0.4 ± 0.2 | 1.3 ± 0.3 | 0.5 ± 0.3 |
| G | 0.5 ± 0.1 | 0.8 ± 0.1 | 2.3 ± 0.2 | 0.9 ± 0.1 | 2.2 ± 0.2 | 0.7 ± 0.1 | 1.1 ± 0.1 | 0.3 ± 0.1 |
| H | 0.5 ± 0.1 | 1.0 ± 0.1 | 2.1 ± 0.3 | 0.6 ± 0.1 | 1.1 ± 0.1 | 0.3 ± 0.1 | 0.6 ± 0.1 | 0.3 ± 0.1 |
| ISO-Oph 137 | ||||||||
| A | – | 21.3 ± 7.9 | 29.6 ± 5.9 | 5.0 ± 1.0 | 10.2 ± 1.1 | 2.5 ± 4.1 | 3.7 ± 2.3 | – |
| B | 0.5 ± 0.1 | 0.9 ± 0.2 | 2.1 ± 0.4 | 0.6 ± 0.2 | 1.2 ± 0.2 | 0.3 ± 0.2 | 1.2 ± 0.2 | 0.5 ± 0.2 |
| C | – | 6.6 ± 1.5 | 12.0 ± 2.0 | 3.0 ± 0.6 | 4.9 ± 0.8 | 1.5 ± 0.6 | 2.1 ± 1.1 | – |
| D | 0.4 ± 0.1 | 0.6 ± 0.1 | 1.5 ± 0.5 | 0.4 ± 0.1 | 0.9 ± 0.1 | 0.3 ± 0.1 | 0.9 ± 0.3 | 0.4 ± 0.3 |
Notes.aValues given for ISO-Oph 21 are uncorrected for extinction since the extinction value could not be estimated.
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