Table 6
Extinction towards each FEL/MHEL region. Line intensities/ratios are measured in a 0.5″ × 0.5″ aperture centred on each source.
Source | C–Ca | H i ratiob | [Fe ii] ratioc | [Fe ii] ratioc | [Fe ii] ratioc | H2 ratiod | H2 excitatione | Publishedf |
Diag | 1.818/2.166 | 1.600/1.712 | 1.664/1.745 | 1.644/1.810 | 2.122/2.424 | diagram | values | |
Av (mag) | Av (mag) | Av (mag) | Av (mag) | Av (mag) | Av (mag) | Av (mag) | Av (mag) | |
|
||||||||
HH 34-IRS | 4 ± 1 | 6.3 ± 1 | 36 ± 8 | 16 ± 1 | 39 ± 2 | 35 ± 5 | 0–6 | > 7.11, 452, 412–323 |
HH 300-IRS | 22 ± 1 | 39 ± 4 | –ve | ... | 61 ± 16 | –ve | 0–27 | ... |
SVS 13 | 10 ± 1 | 9.7 ± 1 | > 128 | ... | < 47 | < 80 | ... | 6–153 |
HH 72-IRS | 10 ± 4 | 4.0 ± 1 | 51 ± 4 | 23 ± 2 | 42 ± 3 | ... | 0 | 4.74 |
HH 999-IRS | 22 ± 3 | 8.2 ± 1 | 62 ± 21 | ... | ... | ... | ... | ... |
HH 26-IRS | 14 ± 2 | ... | > 80 | ... | < 54 | 38 ± 6 | 17–27 | 372 |
HH 83-IRS | 15 ± 2 | ... | ... | ... | ... | ... | ... | ... |
Notes.
Av estimates derived by de-reddening J − H, H − Ks colours of each source in a near-IR colour–colour diagram (Fig. 10).
Extinction towards the H i recombination region at the base of each outflow, assuming case B recombination theory for ne = 109 cm-3, Te = 2000 K (Hummer & Storey 1987): Av = −69.44 × log (1.25 × [I(9 − 4)/IBrγ] ).
Extinction towards the FEL region at the jet base. Values are calculated from three pairs of lines: Av = −132 × log (0.262 × [I1.600/I1.712]), Av = −208 × log (0.499 × [I1.664/I1.745]), and Av = −104 × log (0.201 × [I1.644/I1.810]).
Extinction towards the H2 emission line (MHEL) region associated with each jet, derived from the ratio of the 1–0 S(1) and 1–0 Q(3) lines: Av = −114 × log (0.704 × [IS1/IQ3] ).
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