Non-equilibrium chemistry and cooling in the diffuse interstellar medium

A. J. Richings, J. Schaye and B. D. Oppenheimer


ISRF; nH, tot = 1 cm-3; Z = 0.1 Zsol


Species log Tmin log Tmax log Tpeak Peak
CII 2.0 3.3 2.0 27.4 %
NII 2.0 2.3 2.0 5.9 %
SiII 2.0 3.8 2.7 22.3 %
SIII 2.9 3.9 3.3 5.9 %
FeII 2.8 3.9 3.6 9.1 %
OII 3.9 4.7 4.1 14.9 %
HI 4.0 5.2 4.4 84.1 %
HeI 4.6 4.7 4.7 6.0 %
CIII 4.6 5.1 4.8 14.0 %
HeII 4.7 6.2 4.9 60.0 %
OIII 4.7 5.2 5.0 9.9 %
CIV 5.0 5.1 5.1 7.5 %
NIV 5.1 5.2 5.2 6.5 %
OIV 5.0 5.5 5.3 28.8 %
OV 5.2 5.6 5.4 38.4 %
OVI 5.4 5.7 5.5 17.0 %
NeV 5.4 5.6 5.5 9.9 %
NeVI 5.5 5.8 5.6 21.0 %
NeVII 5.6 5.8 5.7 11.7 %
FeVIII 5.6 5.9 5.8 7.5 %
MgVII 5.8 5.9 5.8 5.5 %
NeVIII 5.8 5.8 5.8 5.5 %
FeIX 5.7 6.1 5.9 20.8 %
MgVIII 5.8 6.0 5.9 7.7 %
FeX 5.9 6.2 6.1 13.4 %
SiIX 6.1 6.1 6.1 5.6 %
FeXII 6.1 6.2 6.2 6.6 %
FeXIII 6.2 6.3 6.2 10.4 %
FeXIV 6.2 6.4 6.3 9.0 %
FeXV 6.3 6.5 6.4 9.6 %
FeXVI 6.4 6.8 6.5 9.7 %
HeIII 5.8 9.0 8.9 25.8 %
HII 2.0 9.0 9.0 73.4 %


Last modified: Fri Mar 21 15:33:10 2014
Email: richings@strw.leidenuniv.nl