Non-equilibrium chemistry and cooling in the diffuse interstellar medium

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


None; nH, tot = 1 cm-3; Z = 0.1 Zsol


Species log Tmin log Tmax log Tpeak Peak
CI 2.0 2.4 2.0 26.7 %
SiII 2.0 2.6 2.3 8.3 %
H2 2.0 4.0 3.6 99.0 %
OI 3.9 4.0 3.9 7.5 %
FeII 3.9 4.0 4.0 6.0 %
HI 3.9 5.9 4.2 98.7 %
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 20.4 %
MgVIII 5.8 6.0 5.9 7.5 %
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 9.3 %
FeXVI 6.4 6.7 6.5 9.4 %
HeIII 5.8 9.0 8.9 25.6 %
HII 5.5 9.0 9.0 72.9 %


Last modified: Fri Mar 21 15:38:21 2014
Email: richings@strw.leidenuniv.nl