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Table 6:

MHD shock model parameters and predicted H2 line fluxesa for 3C 326.
$n_{\rm H}$b $V_{\rm s}$c H2 line fluxes [10-18 W m-2] $\cal{F}_{\rm H_2}$d $\cal{F}_{\rm bol}$e
[cm-3] $\rm [km~s^{-1}]$ S(0) S(1) S(2) S(3) S(4) S(5) S(6) S(7)
104 4 0.74 4.51 0.18 $6.1 \times 10^{-3}$ $3 \times 10^{-4}$ $8.6 \times 10^{-4}$ $2.9 \times 10^{-4}$ $7.5 \times 10^{-4}$ 5.43 13.02
15 0.09 3.22 3.19 10.36 1.35 0.68 0.02 $2.2 \times 10^{-3}$ 18.92 20.55
34 $4.2 \times 10^{-3}$ 0.19 0.29 2.32 1.38 5.33 1.58 2.99 14.09 16.35
Sum 0.84 7.92 3.66 12.69 2.73 6.01 1.60 2.99 38.44 49.92
103 4 1.61 3.74 0.018 $1.3 \times 10^{-3}$ $4.3 \times 10^{-4}$ $1.2 \times 10^{-3}$ $4 \times 10^{-4}$ 10-3 5.37 10.6
24 0.08 3.01 2.44 5.09 0.46 0.17 $7 \times 10^{-3}$ $6.6 \times 10^{-3}$ 11.3 11.6
40 0.02 1.01 1.32 7.57 2.73 5.24 0.68 0.56 19.13 20.07
Sum 1.71 7.75 3.78 12.66 3.2 5.42 0.68 0.56 35.77 42.27
Spitzer Obs. $2.0 \pm 0.3$ $7.5 \pm 0.5$ $4.1 \pm 0.4$ $12.6 \pm 0.4$ $3.1 \pm 0.6$ $5.0 \pm 2.5$ $2.5 \pm 1.0$ $2.9 \pm 1.0$ $39.7 \pm 2.3$  

Notes. (a) This table lists the shock model velocities, the predicted H2 rotational line fluxes, and bolometric luminosities associated with each shock velocity components. Measured H2 fluxes are taken from Ogle et al. (2010,2007). (b) Preshock hydrogen density. (c) MHD shock velocity. (d) Sum of the $\rm H_2$ S(0) to S(7) rotational lines in 10-18 W m-2. (e) Sum over all the lines (bolometric luminosity of the shock).


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