Non-equilibrium chemistry and cooling in the diffuse interstellar medium

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


ISRF10; nH, tot = 10-2 cm-3; Z = Zsol


Species log Tmin log Tmax log Tpeak Peak
OIII 2.0 5.2 2.1 68.3 %
SIII 2.2 2.7 2.4 6.6 %
OIV 2.3 5.5 3.3 44.6 %
SIV 2.7 4.2 3.5 12.8 %
CIV 4.1 5.2 4.4 27.0 %
CIII 4.3 5.1 4.7 24.1 %
HeII 5.0 5.1 5.1 5.4 %
NIV 4.5 5.3 5.1 10.1 %
OV 4.7 5.6 5.4 48.8 %
OVI 5.4 5.7 5.5 23.6 %
NeV 3.2 5.7 5.5 13.9 %
NeVI 5.5 5.8 5.6 30.9 %
MgVI 5.6 5.7 5.7 5.7 %
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 11.5 %
SiVIII 5.9 6.1 6.0 6.1 %
FeX 5.9 6.2 6.1 21.3 %
SiIX 6.0 6.2 6.1 9.3 %
SiX 6.1 6.2 6.2 7.5 %
FeXII 6.1 6.3 6.2 11.6 %
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 19.4 %
OVIII 6.4 7.0 6.6 11.5 %
FeXVI 6.3 6.9 6.6 26.1 %
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 15:20:13 2014
Email: richings@strw.leidenuniv.nl