Non-equilibrium chemistry and cooling in the diffuse interstellar medium

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


None; nH, tot = 10-2 cm-3; Z = Zsol


Species log Tmin log Tmax log Tpeak Peak
CI 2.0 4.1 2.0 27.0 %
SiII 2.0 4.0 2.4 66.1 %
H2 2.0 4.0 3.5 20.6 %
OI 2.9 4.0 3.6 8.7 %
FeII 2.1 4.1 3.8 41.0 %
MgII 3.9 4.1 4.0 7.7 %
HI 3.9 9.0 4.2 91.7 %
CII 2.0 4.8 4.6 12.3 %
OII 4.4 4.8 4.6 15.8 %
SiIII 4.5 4.8 4.7 10.1 %
CIII 4.6 5.1 4.8 30.9 %
HeII 4.7 5.2 4.9 18.9 %
OIII 4.7 5.3 5.0 20.3 %
CIV 4.9 5.2 5.1 14.0 %
NIV 5.1 5.3 5.2 10.0 %
OIV 5.0 5.5 5.2 40.7 %
OV 5.2 5.6 5.4 48.2 %
OVI 5.4 5.7 5.5 23.0 %
NeV 5.3 5.7 5.5 13.9 %
NeVI 5.5 5.8 5.6 30.1 %
MgVI 5.6 5.7 5.7 5.6 %
NeVII 5.6 5.9 5.7 16.4 %
FeVIII 5.6 6.0 5.8 10.6 %
MgVII 5.7 5.9 5.8 7.8 %
NeVIII 5.8 5.9 5.8 7.8 %
FeIX 5.7 6.2 5.9 29.7 %
MgVIII 5.8 6.0 5.9 11.0 %
SiVIII 5.9 6.0 6.0 5.8 %
FeX 5.9 6.2 6.1 20.2 %
SiIX 6.0 6.2 6.1 8.8 %
SiX 6.1 6.2 6.2 7.1 %
FeXII 6.1 6.3 6.2 10.9 %
FeXIII 6.1 6.4 6.2 17.4 %
SiXI 6.2 6.3 6.2 5.4 %
FeXIV 6.2 6.5 6.3 15.4 %
OVII 6.2 6.5 6.4 7.8 %
FeXV 6.2 6.7 6.4 18.0 %
OVIII 6.4 6.9 6.6 10.3 %
FeXVI 6.3 6.9 6.6 23.3 %
FeXVII 6.6 6.9 6.8 9.5 %
FeXVIII 6.8 7.0 6.9 7.9 %
FeXIX 6.9 7.0 7.0 6.4 %
FeXX 7.0 7.1 7.0 6.3 %
FeXXI 7.0 7.2 7.1 6.3 %
FeXXII 7.1 7.3 7.2 8.2 %
FeXXIII 7.1 7.4 7.3 7.8 %
FeXXIV 7.3 7.6 7.4 6.2 %
FeXXV 7.7 8.0 7.8 5.8 %
HeIII 6.6 9.0 9.0 25.8 %
HII 6.2 9.0 9.0 60.8 %


Last modified: Fri Mar 21 15:27:23 2014
Email: richings@strw.leidenuniv.nl