Table C.1: Predicted far-IR ( $\lambda_{\rm peak}\gtrsim15~\mu{\rm m}$) emission spectrum of one molecule of neutral naphthalene (C10H8) in different exciting RFs. Under optically thin conditions total fluxes can be obtained simply multiplying these fluxes by the appropriate column density.
  Integrated flux

 		   Red IRAS
Peak ISRF Rectangle 21282+5050
($\mu$m) (W  sr-1) (%) (W  sr-1) (%) (W  sr-1) (%)

$\parallel$ 15.82		 $1.6 \times 10^{-29}$ (0.51) $2.5 \times 10^{-28}$ (0.62) $1.4 \times 10^{-24}$ (0.48)
[15.90] $4.3 \times 10^{-30}$ (0.14) $7.3 \times 10^{-29}$ (0.18) -
[19.50] $5.4 \times 10^{-30}$ (0.18) $9.7\times 10^{-29}$ (0.24) -
[19.54] $5.4 \times 10^{-30}$ (0.18) $9.4 \times 10^{-29}$ (0.23) -
$\perp$ 20.88 $4.7 \times 10^{-29}$ (1.53) $7.5 \times 10^{-28}$ (1.83) $4.1\times 10^{-24}$ (1.45)
[21.16] $6.0\times 10^{-30}$ (0.20) $1.0 \times 10^{-28}$ (0.25) -
[25.75] $7.3\times 10^{-30}$ (0.24) $1.3 \times 10^{-28}$ (0.31) -
$\parallel$ 27.74 $9.1 \times 10^{-30}$ (0.30) $1.6 \times 10^{-28}$ (0.40) $6.6\times 10^{-25}$ (0.23)
[53.95] $1.1 \times 10^{-29}$ (0.36) $1.8 \times 10^{-28}$ (0.43) -
$\perp$ 58.56 $1.2 \times 10^{-29}$ (0.39) $2.0 \times 10^{-28}$ (0.49) $4.9\times 10^{-25}$ (0.17)


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