Open Access
Table D.1
Range of total H2 luminosities obtained assuming the extinction range indicated, Tex = 2400–2700 K, LTE conditions, and isotropic emission (scaled to a distance of 910 pc). The listed knots can be identified in Fig. 2.
| Lower limit | Upper limit | |||
|---|---|---|---|---|
Knot(a) (10–3 L⊙) |
AV (mag) |  (10–3 L⊙) |
AV (mag) | |
| HH 593A | 5.02 ± 0.07 | 5 | 11.5±0.1 | 10 |
| HH 593B | 6.09 ± 0.09 | 5 | 11.9±0.1 | 10 |
| HH 593C | 4.36 ± 0.07 | 5 | 8.5±0.1 | 10 |
| HH 593D | 6.04± 0.10 | 5 | 11.8±0.1 | 10 |
| A1 | 13.40 ± 0.15 | 5 | 26.4±0.3 | 10 |
| A2 | 3.97 ± 0.12 | 5 | 7.8 ± 0.1 | 10 |
| A3 | 4.78 ± 0.09 | 5 | 9.4±0.1 | 10 |
| A4 | 9.1 ± 0.1 | 5 | 18.0±0.3 | 10 |
| A5 | 7.2 ± 0.1 | 5 | 14.0 ± 0.3 | 10 |
| A6 | 3.9 ± 0.1 | 5 | 7.5 ± 0.3 | 10 |
| A7 | 17.7 ± 0.1 | 5 | 34.7 ± 0.3 | 10 |
| A8 | 3.9 ± 0.1 | 5 | 7.7 ± 0.3 | 10 |
| A9 | 5.0 ± 0.1 | 5 | 9.7 ± 0.3 | 10 |
| A10 | 9.7 ± 0.1 | 5 | 19.0±0.3 | 10 |
| A11 | 14.1 ± 0.3 | 5 | 27.5 ± 0.4 | 10 |
| A12 | 14.1 ± 0.1 | 5 | 27.5 ± 0.3 | 10 |
| A13 | 3.30 ± 0.09 | 5 | 6.5 ± 0.1 | 10 |
| A14 | 7.9 ± 0.1 | 5 | 15.5±0.3 | 10 |
| A15 | 28.0 ± 0.1 | 5 | 54.6 ± 0.3 | 10 |
| B1 | 13.0 ± 0.3 | 5 | 25.5 ± 0.4 | 10 |
| B2 | 37.8 ± 0.3 | 5 | 74.2 ± 0.6 | 10 |
| B3 | 12.2 ± 0.1 | 5 | 24.0 ± 0.3 | 10 |
| B4 | 36.2 ± 0.3 | 5 | 71.0±0.4 | 10 |
| B5 | 55.9 ± 0.3 | 5 | 109.5±0.4 | 10 |
| B6 | 19.4± 0.1 | 5 | 38.1 ± 0.3 | 10 |
| B7 | 28.0 ± 0.1 | 5 | 54.8 ± 0.3 | 10 |
| B8 | 53.7 ± 0.3 | 5 | 105.4±0.4 | 10 |
| B9 | 5.0 ± 0.1 | 5 | 9.7 ± 0.1 | 10 |
| B10 | 5.9 ± 0.1 | 5 | 11.6±0.3 | 10 |
| B11 | 5.8 ± 0.1 | 5 | 11.3±0.1 | 10 |
| C1 | 0.91 ± 0.07 | 0 | 1.3±0.1 | 2 |
| C2 | 1.74± 0.04 | 0 | 2.50±0.06 | 2 |
| C3 | 1.47 ± 0.04 | 0 | 2.12±0.07 | 2 |
| C4 | 1.65 ± 0.06 | 0 | 2.34±0.07 | 2 |
| C5 | 7.26 ± 0.04 | 0 | 10.41 ± 0.06 | 2 |
| C6 | 13.57 ± 0.04 | 0 | 19.49 ± 0.06 | 2 |
| C7 | 18.21 ± 0.06 | 0 | 26.13±0.07 | 2 |
| C8 | 18.42 ± 0.06 | 0 | 26.46±0.09 | 2 |
| C9 | 5.02 ± 0.06 | 0 | 7.23 ± 0.09 | 2 |
| C10 | 14.84 ± 0.07 | 0 | 21.30±0.09 | 2 |
| C11 | 15.18 ± 0.07 | 0 | 21.8±0.1 | 2 |
| C12 | 10.73 ± 0.06 | 0 | 15.40 ± 0.07 | 2 |
| C13 | 16.77 ± 0.07 | 0 | 24.06±0.09 | 2 |
| C14 | 26.65 ± 0.06 | 0 | 38.29 ± 0.07 | 2 |
| C15 | 4.95 ± 0.09 | 0 | 7.1 ± 0.1 | 2 |
| C16 | 19.26 ± 0.07 | 0 | 27.7 ± 0.1 | 2 |
| C17 | 2.9 ± 0.4 | 0 | 4.1 ± 0.6 | 2 |
| G1 | 1.24± 0.03 | 2 | 3.3 ± 0.1 | 10 |
| G2 | 2.91 ± 0.04 | 2 | 7.8 ± 0.1 | 10 |
| G3 | 9.01 ± 0.07 | 2 | 24.1 ± 0.1 | 10 |
| G4 | 3.37 ± 0.06 | 2 | 9.0 ± 0.1 | 10 |
| G5 | 1.09 ± 0.03 | 2 | 2.94±0.09 | 10 |
| G6 | 2.00 ± 0.06 | 2 | 5.3 ± 0.1 | 10 |
| G7 | 3.74± 0.09 | 2 | 10.0±0.1 | 10 |
| O1 | 5.78 ± 0.1 | 7 ± 2 | … | … |
Notes.(a)Following the notation used in Beltrán et al. (2009).
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