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 = 0.1 Zsol


Species log Tmin log Tmax log Tpeak Peak
SiII 2.2 2.7 2.4 7.2 %
OIII 2.0 5.2 2.6 28.2 %
SIII 2.2 4.1 2.8 11.6 %
SIV 3.3 3.4 3.3 5.0 %
SiIII 4.3 4.8 4.5 9.7 %
HI 4.3 4.9 4.6 12.1 %
CIII 4.2 5.1 4.7 30.6 %
HeII 4.7 6.2 5.0 48.0 %
CIV 5.0 5.1 5.1 7.7 %
NIV 5.1 5.2 5.2 6.7 %
OIV 3.1 5.5 5.3 29.1 %
OV 5.2 5.6 5.4 38.8 %
OVI 5.4 5.7 5.5 17.2 %
NeV 5.4 5.6 5.5 10.0 %
NeVI 5.5 5.8 5.6 21.3 %
NeVII 5.6 5.8 5.7 11.9 %
FeVIII 5.6 5.9 5.8 7.6 %
MgVII 5.8 5.9 5.8 5.5 %
NeVIII 5.8 5.8 5.8 5.6 %
FeIX 5.7 6.1 5.9 21.1 %
MgVIII 5.8 6.0 5.9 7.8 %
FeX 5.9 6.2 6.1 13.5 %
SiIX 6.1 6.1 6.1 5.7 %
FeXII 6.1 6.2 6.2 6.7 %
FeXIII 6.2 6.3 6.2 10.5 %
FeXIV 6.2 6.4 6.3 9.0 %
FeXV 6.3 6.5 6.4 9.7 %
FeXVI 6.4 6.8 6.5 9.8 %
HII 2.0 9.0 8.6 72.9 %
HeIII 3.6 9.0 8.9 25.6 %


Last modified: Fri Mar 21 15:23:40 2014
Email: richings@strw.leidenuniv.nl