Non-equilibrium chemistry and cooling in the diffuse interstellar medium

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


ISRF; nH, tot = 10-2 cm-3; Z = Zsol


Species log Tmin log Tmax log Tpeak Peak
CII 2.0 2.2 2.0 12.2 %
NII 2.0 2.1 2.0 6.5 %
SiII 2.0 2.9 2.3 13.5 %
NIII 2.0 4.9 2.4 6.2 %
OIII 2.0 5.3 2.5 48.2 %
SIII 2.0 4.3 2.8 19.9 %
SIV 3.0 4.0 3.4 9.7 %
SiIII 4.2 4.8 4.5 13.1 %
CIII 4.1 5.1 4.7 40.1 %
HeII 4.8 5.2 5.0 11.3 %
CIV 4.3 5.2 5.1 13.8 %
NIV 5.0 5.3 5.2 10.2 %
OIV 2.9 5.5 5.2 41.3 %
OV 5.2 5.6 5.4 49.0 %
OVI 5.4 5.7 5.5 23.7 %
NeV 5.3 5.7 5.5 14.3 %
NeVI 5.5 5.8 5.6 31.2 %
MgVI 5.6 5.7 5.7 5.8 %
NeVII 5.6 5.9 5.7 17.0 %
FeVIII 5.6 6.0 5.8 11.0 %
MgVII 5.7 5.9 5.8 8.1 %
NeVIII 5.7 5.9 5.8 8.2 %
FeIX 5.7 6.2 5.9 31.0 %
MgVIII 5.8 6.0 5.9 11.4 %
SiVIII 5.9 6.1 6.0 6.1 %
FeX 5.9 6.2 6.1 21.2 %
SiIX 6.0 6.2 6.1 9.2 %
SiX 6.1 6.2 6.2 7.5 %
FeXII 6.1 6.3 6.2 11.5 %
FeXIII 6.1 6.4 6.2 18.5 %
SiXI 6.2 6.3 6.2 5.7 %
FeXIV 6.2 6.5 6.3 16.4 %
OVII 6.2 6.5 6.4 8.3 %
FeXV 6.2 6.7 6.4 19.3 %
OVIII 6.4 7.0 6.6 11.5 %
FeXVI 6.3 6.9 6.6 26.0 %
FeXVII 6.6 6.9 6.8 11.0 %
FeXVIII 6.8 7.0 6.9 9.2 %
FeXIX 6.9 7.1 7.0 7.5 %
FeXX 7.0 7.1 7.0 7.3 %
FeXXI 7.0 7.2 7.1 7.4 %
FeXXII 7.1 7.3 7.2 9.5 %
FeXXIII 7.1 7.4 7.3 9.2 %
FeXXIV 7.3 7.6 7.4 7.3 %
FeXXV 7.6 8.0 7.8 6.6 %
HeIII 6.5 9.0 8.9 27.4 %
HII 2.0 9.0 9.0 64.6 %


Last modified: Fri Mar 21 15:22:55 2014
Email: richings@strw.leidenuniv.nl