Table 6
Summary of the brightness decomposition of lines with disk-like profile.
| Species/λ0 | Aki | Ek | vrad | Vp2p | FWHM | Notes |
|---|---|---|---|---|---|---|
| (Å) | (s−1) | (eV) | (km s−1) | (km s−1) | (km s−1) | |
| FeI 5506.8 | 1.14E+08 | 3.241 | 26.9 ± 0.3 | 78 ± 6 | 113 ± 23 | Blue-dominated, no high-velocity wings. |
| FeI 5572.8 | 2.28E+07 | 5.621 | 35.8 ± 0.3 | 72 ± 4 | 115 ± 2 | Very disky, no high-velocity wings, some central emission. |
| CaI 5598.5 | 4.30E+07 | 4.735 | 21.3 ± 0.6 | 81 ± 2 | 113 ± 3 | Small blue wings. |
| FeI 5615.6 | 2.39E+05 | 5.539 | 26.2 ± 0.1 | 62 ± 1 | 120 ± 1 | Strong high-velocity wings. |
| FeI 5624.5 | 8.30E+05 | 5.621 | 30.2 ± 0.1 | 74 ± 2 | 105 ± 2 | Strong blue high-velocity wing. |
| FeI 6065.5 | 1.07E+06 | 4.652 | 31 ± 1 | 74 ± 2 | 119 ± 3 | Strong high-velocity wings, mostly blue. |
| NiI 6108.1 | 1.30E+05 | 3.706 | 24.5 ± 0.8 | 55 ± 3: | 95 ± 2 | Very asymmetric, red side may be absorbed by nearby feature. |
| FeI 6256.4 | 7.40E+04 | 4.435 | 30 ± 3 | 87 ± 1 | 108 ± 11 | Disk-like, but has low S/N and nearby absorption lines. |
| FeI 6265.1 | 6.84E+04 | 4.154 | 36.9 ± 0.1 | 76 ± 4 | 108 ± 2 | Clean, no wings. |
| FeI 6358.6 | 5.19E+05 | 6.092 | 36 ± 1 | 81 ± 5 | 107 ± 14 | Low S/N and asymmetric continuum due to nearby lines. |
| FeI 6393.6 | 4.81E+05 | 4.371 | 23.5 ± 0.5 | 62 ± 2 | 115 ± 1 | Asymmetric, may have an additional blueshifted absorption. |
| FeI 6400.0 | 9.27E+06 | 5.539 | 37.5 ± 0.3 | 79 ± 2 | 118 ± 2 | High-velocity wings. |
| FeI 6411.6 | 4.43E+06 | 5.587 | 41 ± 1 | 82 ± 17 | 107 ± 15 | Red-dominated. |
| FeI 6421.4 | 3.04E+05 | 4.209 | 29.1 ± 0.3 | 73 ± 22 | 109 ± 2 | |
| CaI 6439.1 | 5.30E+07 | 4.103 | 27 ± 1 | 82.5 ± 0.8 | 111 ± 15 | Blue-dominated, very strong high-velocity blue wing. |
| FeI 6462.7 | 5.60E+04 | 4.371 | 25.9 ± 0.6 | 75 ± 2 | 113 ± 2 | |
| CaI 6717.7 | 1.20E+07 | 4.554 | 27.4 ± 0.9 | 74 ± 2 | 124 ± 4 | Asymmetric continuum. |
| FeI 6750.2 | 1.17E+05 | 4.260 | 25 ± 0.1 | 80 ± 1 | 107 ± 17 | Very extended high-velocity wings to red and blue parts. |
| NiI 6767.8 | 3.30E+05 | 3.658 | 27.9 ± 0.8 | 79 ± 1 | 109 ± 2 | Blue high-velocity wing. |
| FeI 8674.7 | 6.17E+05 | 4.260 | 37.6 ± 0.6 | 78 ± 2 | 108 ± 4 | Flat-top. |
| FeI 8824.2 | 3.53E+05 | 3.603 | 31.1 ± 0.3 | 68 ± 1 | 121 ± 2 | High-velocity wings, central narrow emission. |
| FeI 8838.4 | 3.83E+05 | 4.260 | 34.9 ± 0.4 | 80.1 ± 0.7 | 114 ± 3 |
Notes. Radial velocity estimate is affected if the line is very asymmetric. If the radial velocity is very much off for any reason, it introduces artificial red/blue asymmetries. Also, if the NIST wavelength has large uncertainties, this may result in uncertain wavelengths and thus a further error in the radial velocity and line asymmetry. The quantity Vp2p indicates the velocity between the double peaks of the line. Lines with potential contamination, blends, or very irregular continuum have been removed from the list.
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