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Table 2:

Quantities relevant to PAH survival.
  (1) (2) (3) (4) (5) (6) (7) (8) (9)

component
$h\overline{\nu}$ $\kappa$ $\eta$ ${K/K_{\rm V}}$ x z0/H $\ell/H$ $t_{\rm abs}$ $v_{\rm cr}$
  eV 10-4 Å2             m/s
photosphere 2.7 700 $\ll$1 1.2 - 4.4 0.5 5 s -
FUV 4.2 700 $\ll$1 1.5 - 4.5 0.5 120 s -
EUV 97 36 $\sim $0.5 110 9 5.3 0.4 9 days 2900
X-ray 1100 0.17 $\ll$1 0.55 100 4.2 0.5 290 yr 3.4

Notes.  $z_0, \ell, t_{\rm abs}$and $v_{\rm cr}$ refer to r=10 AU.
(1) The mean energy of destructive photons $h\overline{\nu}$ from Eq. (5) at the bottom of the extinction layer (see Fig. 5); for photospheric and FUV photons we put $\nu_{\rm c} =0$and for EUV and X-rays we integrate for $\nu \geq
\nu_{\rm c}$ (Eq. (10)); (2) absorption cross section $\kappa$ per C atom at a frequency $\overline{\nu}$; (3) approximate mean degree of ionization of the gas in the extinction layer ; (4) extinction cross section of gas and dust at frequency $\overline{\nu}$normalized to $K_{\rm V}= 200$ cm2 g-1; (5) number of expelled atoms x per absorption event from Eq. (14); (6) altitude of the bottom of the extinction layer in units of the scale height H; (7) thickness of extinction layer; (8) mean time $t_{\rm abs}$ from Eq. (4) in which one photon is absorbed; (9) critical vertical velocity for PAH survival.


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