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Table 6

Excitation temperature, extinction, and reduced χ2from fits to the H2lines (plus AVfrom [Fe ii] line ratios).

Knot(a) Tex (K) AV (mag) Reduced χ2
HK + JH band (b)

C6 2305 ±180 5±3 0.2
C7 2417 ±15 0 ± 0.3 21
C10 south 2734 ± 27 0 ± 0.3 12
C12 north 2632 ± 19 0 ± 0.3 39
C14 2266 ± 10 0 ± 0.2 146
C16 north 2336 ± 31 6.3 ± 0.5 35

HK band(b)

C17 north 1292 ±239 0±4 1

JH band (b)

C15 3589 ±221 1.2 ± 0.7 5
A7(c) 9±3
A11(c) 5±2
A12(c) 7±2
O1(c) 7±2

KB grism band(b)(d)

C8 2215 ± 42 14±1 15
C10 2246 ± 29 19±1 11
east of C8–C10 2278 ± 89 4.4 ± 2.4 0.2
north-east of C14 2182 ± 59 21 ± 2 5
C14 2241 ± 31 14±1 5
A7(e) 2089 ± 124 0±8 0.4
A15(e) 2425 ± 137 0±9 0.05
B8 2617 ± 285 22 ± 18 0.3
G1(e) 2240 ± 275 16±11 3
G2(e) 2331 ± 268 7±12 0.2
G3(e) 2249 ± 72 0±9 0.3
G4(e) 2405 ± 145 5±11 0.4

Notes. The listed knots can be identified in Fig. 2.(a)Following the notation used inBeltrán et al. (2009).(b)Spectra spanning the indicated band. (c)AV from 1.644/1.257 μm [Fe ii] line ratios. (d)Fits in this band underestimate Tex and overestimate AV (see text). (e)H2 1–0 S(3) line point at 1.957 μm not included in the fit to obtain a consistent result.

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