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 = 0.1 Zsol


Species log Tmin log Tmax log Tpeak Peak
OIII 2.0 5.2 2.3 31.1 %
SIV 2.9 3.9 3.4 6.9 %
CIV 4.2 5.1 4.5 20.5 %
CIII 4.4 5.0 4.7 19.9 %
HeII 4.8 6.2 5.1 30.0 %
NIV 4.6 5.2 5.1 7.0 %
OIV 2.4 5.5 5.2 28.4 %
OV 4.7 5.6 5.4 39.2 %
OVI 5.4 5.7 5.5 17.5 %
NeV 5.4 5.6 5.5 9.8 %
NeVI 5.5 5.8 5.6 21.4 %
NeVII 5.6 5.8 5.7 12.0 %
FeVIII 5.6 5.9 5.8 7.7 %
MgVII 5.8 5.9 5.8 5.6 %
NeVIII 5.8 5.8 5.8 5.6 %
FeIX 5.7 6.1 5.9 21.2 %
MgVIII 5.8 6.0 5.9 7.8 %
FeX 5.9 6.2 6.1 13.6 %
SiIX 6.0 6.1 6.1 5.7 %
FeXII 6.1 6.2 6.2 6.7 %
FeXIII 6.2 6.3 6.2 10.6 %
FeXIV 6.2 6.4 6.3 9.1 %
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 2.4 9.0 8.9 25.6 %


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