12/30/10 1 Ab initio spectral simulations
Detailed microphysics Energetic radiation &
particles interact with gas
Ejected electrons heats,
excite & ionize gas
Ionization drives
chemistry
Kinetic temperature,
ionization, full spectrum, predicted
The nH – Tu plane
Θ
1 Ori
exciting stars Ionized gas Atomic gas Veil Molecular gas
100” BN 0.5 pc
A A B B OMC, 13CO To Earth Figure 8.4, Osterbrock & Ferland AGN3
Depth (cm)
1.5e+17 1.6e+17 1.7e+17 1.8e+17 1.9e+17 2.0e+17
molecular fractional
10-4 10-3 10-2 10-1 100
Temperature
100 1000 10000
- log fractional ionization
1 2 He0 He+ C+2 H2 C0 H+ H0 CH CO OH H2O H2O
Ferland, G.J., 2003, ARA&A, 41, 517
Carbon ionization along ray
Depth (cm)
1e+15 1e+16 1e+17 1e+18
Ion - molecular fraction
- 8
- 6
- 4
- 2
C+3 C0 C+ C+2 CO
Spectrum at half-H2 point
1.00E-02 1.00E-01 1.00E+00 1.00E+01 1.00E+02 1.00E+03 1.00E+04 1.00E-01 1.00E+00 1.00E+01 1.00E+02 1.00E+03
Wavelength (microns) νSν (erg cm-2 s-1)