Non-equilibrium chemistry and cooling in the diffuse interstellar medium

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


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


Species log Tmin log Tmax log Tpeak Peak
CII 2.0 3.7 2.0 56.9 %
SiII 2.0 3.9 2.6 46.3 %
H2 3.2 3.8 3.5 13.8 %
FeII 2.3 4.0 3.8 30.4 %
SII 3.8 4.0 3.9 7.7 %
HI 3.9 5.8 4.2 98.5 %
HeI 4.5 4.7 4.6 8.6 %
OII 4.6 4.7 4.7 5.8 %
CIII 4.6 5.1 4.8 13.4 %
HeII 4.7 6.2 4.9 60.0 %
OIII 4.8 5.2 5.0 9.8 %
CIV 5.0 5.1 5.1 7.4 %
NIV 5.1 5.2 5.2 6.5 %
OIV 5.0 5.5 5.3 28.6 %
OV 5.2 5.6 5.4 38.1 %
OVI 5.4 5.7 5.5 16.8 %
NeV 5.4 5.6 5.5 9.7 %
NeVI 5.5 5.8 5.6 20.7 %
NeVII 5.6 5.8 5.7 11.5 %
FeVIII 5.6 5.9 5.8 7.4 %
MgVII 5.8 5.8 5.8 5.4 %
NeVIII 5.8 5.8 5.8 5.4 %
FeIX 5.7 6.1 5.9 20.5 %
MgVIII 5.8 6.0 5.9 7.6 %
FeX 5.9 6.2 6.1 13.1 %
SiIX 6.1 6.1 6.1 5.5 %
FeXII 6.1 6.2 6.2 6.5 %
FeXIII 6.2 6.3 6.2 10.2 %
FeXIV 6.2 6.4 6.3 8.7 %
FeXV 6.3 6.5 6.4 9.4 %
FeXVI 6.4 6.7 6.5 9.5 %
HeIII 5.8 9.0 8.9 25.7 %
HII 2.0 9.0 9.0 73.2 %


Last modified: Fri Mar 21 15:35:53 2014
Email: richings@strw.leidenuniv.nl