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Table 5

Strong lines used to derive the accretion properties.

Species λ E i E k A ki Notes
(Å) (eV) (eV) (s-1)

Fe I 4375.930 0 2.83 2.95E+04 F
Fe I 4461.652 0.08 2.87 2.95E+04 F
Fe I 4482.169 0.11 2.88 2.09E+04
Ti II 4571.980 1.57 4.28 1.92E+07 F
Fe I 4602.941 1.48 4.18 1.72E+05 F
Fe II 4923.921 2.89 5.41 4.28E+06 F, BA
Fe II 5018.434 2.89 5.36 2.00E+06 F, BA
Fe I 5060.034 4.3 6.75
Fe I 5083.338 0.95 3.4 4.06E+04
Fe I 5110.358 3.57 6.0 9.99E+05
Ti II 5129.150 1.89 4.31 1.46E+06 F
Mg I 5167.32 1.48 3.88 2.72E+06 F, BA
Mg I 5172.684 2.71 5.11 3.37E+07 F
Fe I 5332.899 1.55 3.88 4.36E+04
Fe I 5341.024 1.6 3.93 5.21E+05
Fe I 5397.127 0.91 3.21 2.58E+04
Fe I 5455.609 1.01 3.28 6.05E+05
Fe I 5506.779 0.99 3.24 5.01E+04 F
Fe I 5916.247 2.45 4.55 2.15E+04
Si II 5957.560 10.06 12.15 5.60E+07
Fe I 5958.333 2.17 4.26
Fe II 5991.376 3.15 5.22 4.20E+03 F
Fe I 6191.558 2.43 4.43 7.41E+05 F
Fe I 6200.312 2.61 4.61 9.06E+04 F
Fe I 6336.824 3.87 5.64 7.71E+06
Si II 6347.100 8.12 10.07 5.84E+07
Fe I 6393.601 2.43 4.37 4.81E+05
Fe I 6400.001 3.6 5.54 9.27E+06 F
Fe I 6421.351 2.28 4.21 3.04E+05
Fe I 6498.939 0.96 2.87 4.64E+02
Hα 6562.57 10.2 12.09 5.39E+07 BA
Fe II 6678.883 10.93 12.79 2.40E+07 F
Fe I 6750.152 2.42 4.26 1.17E+05
Fe I 6978.851 2.48 4.26 1.44E+05
Fe I 8048.990 4.14 5.68
H I 8467.26 12.1 13.55 3.44E+03
Ca II 8498.020 1.69 3.15 1.11E+06 F
Fe I 8514.07 2.19 3.65 1.09E+05
Ca II 8542.09 1.69 3.15 9.90E+06
Ca II 8662.140 1.69 3.12 1.06E+07
Mg I 8806.756 4.36 5.75 1.27E+07
Fe I 8824.221 2.19 3.6 3.53E+05 F

Notes. The “Notes” indicate whether a blue-shifted absorption is present (BA) and whether the line was fitted for the velocity analysis (F).

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