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Home All issues Volume 501 / No 3 (July III 2009) A&A, 501 3 (2009) 973-983 Full HTML
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Table 5:

Line list of 42 Fe  I lines used for the analysis of the ONC stars along with excitation potential ($\chi $), $\log~gf$ values, equivalent widths measured on the solar spectrum acquired with UVES and corresponding Fe abundances.
$\lambda $ $\chi $ $\log~gf$ $EW_{\odot}$ $\log~n$(Fe)$_{\odot}$
(Å) (EV)   (mÅ)  
6703.576 2.760 -3.100 37 7.53
6713.745$^{\rm w}$ 4.790 -1.410 23 7.50
6726.673$^{\rm w}$ 4.610 -1.050 48 7.50
6750.164 2.420 -2.655 75 7.51
6786.860 4.190 -1.900 26 7.49
6806.856 2.730 -3.140 36 7.51
6810.267 4.610 -1.000 50 7.49
6820.374$^{\rm w}$ 4.640 -1.160 41 7.51
6839.835 2.560 -3.450 29 7.50
6843.655$^{\rm w}$ 4.550 -0.860 63 7.53
6858.155 4.610 -0.950 52 7.48
6862.496$^{\rm w}$ 4.560 -1.430 33 7.53
6945.200 2.420 -2.460 81 7.41
6951.250 4.560 -1.050 52 7.52
6978.860$^{\rm w}$ 2.480 -2.490 84 7.56
6988.530 2.400 -3.420 39 7.51
7022.960 4.190 -1.110 67 7.51
7024.070$^{\rm w}$ 4.070 -1.940 30 7.49
7038.230$^{\rm w}$ 4.220 -1.130 62 7.47
7083.400$^{\rm w}$ 4.910 -1.260 24 7.48
7142.520$^{\rm w}$ 4.950 -0.930 39 7.51
7219.690 4.070 -1.570 50 7.52
7221.210 4.560 -1.220 42 7.49
7228.700$^{\rm c}$ 2.760 -3.270 27 7.45
7284.840 4.140 -1.630 43 7.51
7306.570 4.180 -1.550 43 7.47
7401.690$^{\rm w}$ 4.190 -1.600 44 7.54
7418.670 4.140 -1.440 51 7.47
7421.560$^{\rm w}$ 4.640 -1.690 20 7.52
7447.400 4.950 -0.950 35 7.44
7461.530$^{\rm c}$ 2.560 -3.450 30 7.49
7491.660 4.300 -1.010 70 7.54
7507.270 4.410 -1.030 62 7.52
7531.150 4.370 -0.640 90 7.58
7547.900$^{\rm w}$ 5.100 -1.110 25 7.51
7568.910 4.280 -0.900 76 7.52
7583.800 3.020 -1.930 85 7.49
7710.363 4.220 -1.112 66 7.48
7751.110$^{\rm w}$ 4.990 -0.740 48 7.50
7807.910$^{\rm w}$ 4.990 -0.510 61 7.50
7912.870 0.860 -4.850 49 7.50
7959.150$^{\rm w}$ 5.030 -1.180 24 7.47
Lines labeled with a ``w'' or ``c'' have been used for the warm
star HD 294297 or for the cool ONC stars only.

Source LaTeX | All tables | In the text

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