Table 3:
Summary of model atoms used in the disk model calculations. For
each ion we list the number of NLTE levels and the number of line
transitions. In brackets we give the number of lines in the wavelength
range covered by our optical spectra after fine-structure splitting for
detailed line-profile calculations.
Element |
Ion |
NLTE levels |
Lines |
H |
I |
10 |
45 (8) |
|
II |
1 |
- |
He |
I |
29 |
61 (16) |
|
II |
14 |
91 (14) |
|
III |
1 |
- |
C |
I |
7 |
4 (0) |
|
II |
38 |
160 (42) |
|
III |
58 |
329 (143) |
|
IV |
9 |
17 (2) |
|
V |
1 |
- |
O |
I |
1 |
- |
|
II |
29 |
82 (56) |
|
III |
36 |
42 (47) |
|
IV |
11 |
5 (0) |
|
V |
6 |
4 (0) |
|
VI |
1 |
- |
Ne |
I |
3 |
0 |
|
II |
68 |
232 (49) |
|
III |
4 |
0 (0) |
|
IV |
1 |
- |
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