Table 1
Parameters of the five N I lines used in the abundance analysis.
Line label | λair ∕nm | Lower | χlow ∕eV | Upper | χup ∕eV | log gf | log(γrad.∕s−1) | ![]() |
αH |
---|---|---|---|---|---|---|---|---|---|
N I 744 | 744.229 | 3s 4P3∕2 | 10.330 | ![]() |
11.996 | − 0.403 | + 8.751 | 530 | 0.2271 |
lN I 822 | 821.633 | 3s 4P5∕2 | 10.336 | ![]() |
11.844 | + 0.138 | + 8.745 | 497 | 0.2286 |
N I 863 | 862.923 | 3s 2P3∕2 | 10.690 | ![]() |
12.126 | + 0.077 | + 8.713 | 576 | 0.2337 |
N I 868 | 868.340 | 3s 4P3∕2 | 10.330 | ![]() |
11.758 | + 0.106 | + 8.740 | 481 | 0.2306 |
N I 1011 | 1010.89 | ![]() |
11.753 | 3d 4F5∕2 | 12.979 | + 0.444 | + 7.773 | 750 | 0.2671 |
Notes. The table lists: wavelengths in air λair; electronic configurations and spectroscopic terms of the lower and upper states, with excitation energies χlow and χup ; oscillator strengths f; natural broadening coefficients γrad. (FWHM in angular frequency units); and ABO broadening cross-sections σH at reference velocity v = 104 m s−1 and exponents αH, such that the cross-section is proportional to v−α (Anstee & O’Mara 1995). Data sources are the same as used to construct the non-LTE model atom (Sect. 2.4); in particular, the transition probabilities were drawn from Tachiev & Froese Fischer (2002).
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