Kaufman, Wolfire, Hollenbach, & Luhman 1999, ApJ
Standard Model Parameters

Parameter Symbol Value
Turbulent Doppler Velocity $\delta v_D$ 1.5$\,\rm km\,s^{-1}$
Carbon abundance$^{\rm a}$ XC $1.4\times 10^{-4}$
Oxygen abundance$^{\rm a}$ XO $3.0\times 10^{-4}$
Silicon abundance$^{\rm a}$ XSi $1.7\times 10^{-6}$
Sulfer abundance$^{\rm a}$ XS $2.8\times 10^{-5}$
Iron abundance$^{\rm a}$ XFe $1.7\times 10^{-7}$
Magnesium abundance$^{\rm a}$ XMg $1.1\times 10^{-6}$
Dust abundance relative to diffuse ISM $\delta_d$ 1
FUV Dust absorption/visual extinction $\delta_{UV}$ 1.8
Dust visual cross section per H $\sigma_{\rm V}$ $5\times 10^{-22}\,\rm cm^{2}$
Formation rate of $\rm H_2$ on dust$^{\rm b}$ Rform $3\times 10^{-17}\,\rm s^{-1}$
PAH abundance $X_{\rm PAH}=n_{\rm PAH}/n$ $4\times 10^{-7}$
Cloud density n $10^1\,{\rm cm^{-3}}\le\,n\,\le\, 10^7\,{\rm cm^{-3}}$
Incident FUV flux G0 $10^{-0.5}\,\le\,G_0\,\le\, 10^{6.5}$
$^{\rm a}$Gas phase abundances relative to H nuclei from Savage & Sembach 1996

$^{\rm b}$Rate cm-3 s-1 given by $R_{form}n_{\rm HI}$


WITS PDRT DIRT UMD IRSA

Please direct comments, criticisms, corrections and contributions to Marc Pound.
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