 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
1. |
Outflow velocities, mass loss (wavelengths)
|
|
|
2. |
Electron temperatures (RRCs)
|
|
|
3. |
Optical depth => column densities
|
|
|
via absorption (oscillator strengths) and emission
|
|
|
4. |
Elemental abundances
|
|
|
(column density behavior as a function of
|
|
|
ionization parameter x = L/ner2)
|
|
5. |
Ionization balance (x), density (ne) and
position (r)
|
|
|
|
|
(photo-ionization and recombination rates, including
|
|
autoionization processes)
|
|
|
Note: C 2 is not a measurable astrophysical
quantity!
|
|