HARPS spectra (R=110000) of the binary system AK_Sco (HD 152404; F5 IVe)
Spectral range: 4000-6912 A

Identification labels:
Interval: 520.2-520.3 nm---->label: 256  26.00 34328  397

256: last 3 digits of wavelengths in nm  lambda=520.2256 nm
26.00 = Fe I  26=atomic number of the element (Fe), 00=charge (I)
34328=lower enrgy level in cm-1
397=per mil residual intensity of isolated line before broadening (rotational + instrumental)
RED LABELS: identifications in the primary BLACK LABELS: identifications in the secondary
Herbig F5 IVe star- Spectroscopic binary. A and B are the primary and the secondary stars. Teff=6500 K from Alencar et al. (2003) A: Star parameters: Teff=6500 K, log g=4.5, vturb=1 km/sec (from spectrum) vsini=18 km/sec from several lines in the spectrum. B: Star parameters: Teff=6500 K, log g=4.5, vturb=2 km/sec (from spectrum) vsini=21 km/sec from several lines in the spectrum. The two components are surrounded by a circumbinary disk which may obscure the liminosity of the secondary. We adopted as luminosty reduction for the B star these percetages from Li 6707 and Sr II 4077 and 4215. phi luminosity percentage 0.946 10 % 0.950 50 % 0.018 50 % 0.025 80 % 0.090 100 % 0.169 100 % Abundances adoted to compute the synthetic spectrum. The abundances of the other elements were assumed to be solar. star A star B sun Li -8.70 [+2.3] -8.50 [+2.5] -10.99 C -3.61 [ 0.0] -3.61 [ 0.0] -3.61 O -3.35 [ 0.0] -3.35 [ 0.0] -3.35 Na -5.93 [-0.1] -5.78+/-0.05 [+0.05] -3.83 Mg -4.55 [-0.1] -4.45 [ 0.0] -4.45 Al -5.61 [ 0.0] -5.61 [ 0.0] -5.61 Si -4.40+/-0.07 [ 0.13] -4.33+/-0.07 [ 0.20] -4.53 S -4.72+/-0.10 [ 0.20] -4.62+/-0.10 [ 0.30] -4.92 Ca -5.70+/-0.10 [ 0.02] -5.84+/-0.08 [-0.12] -5.72 Sc -8.98 [-0.1 ] -8.68 [ 0.20] -8.88 Ti -6.96+/-0.15 [ 0.15] -7.14+/-0.09 [-0.03] -7.11 V -8.15 [ 0.0] -8.15 Cr -6.34+/-0.17 [ 0.08] -6.39+/-0.02 [+0.03] -6.42 Mn -6.62 [ 0.00] -6.62 [+0.00] -6.62 Fe -4.62+/-0.16 [-0.05] -4.49+/-0.15 [+0.08] -4.57 Co -6.91 [+0.20] -7.11 Ni -5.84+/-0.08 [ 0.00] -5.74+/-0.17 [+0.14] -5.84 Cu -7.86 [ 0.00] -7.86 [+0.00] -7.86 Zn -7.38 [ 0.10] -7.58 [-0.10] -7.48 Sr -9.10 [+0.11] -8.95+/-0.05 [+0.24] -9.21 Y -9.40 [+0.40] -9.50 [+0.30] -9.83 Zr -9.05 [+0.40] -9.45 [ 0.00] -9.45 Ba -9.51 [+0.28] -9.41 [+0.38] -9.79 La -10.22+/-0.15 [+0.70] -10.57 [+0.36] -10.93 Ce -10.46 [ 0.00] -10.46
Comparison of the observed and computed spectra at the phase 0.090
 Phases  ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169


Comparison of special lines at different phases

 Halpha    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Hbeta    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Hgamma    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Hdelta    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 He I 5875.61  the observed spectra  ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Li I (6708 A)    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Na I (5889.95 + 5895.92)    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Ca I (6122.217 A)  at all the phases:red line A, black line B  ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Ca II K (3933 A)    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Ca II H + Heps (3968.47+3970.074 A)    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Mg I 5183.604 A  the observed spectra  ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Fe I 5615.644 A    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Fe II 5018.436 A  the observed spectra  ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Sr II 4077 A)    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169
 Sr II 4215 A)    ph_0.946  ph_0.950  ph_0.018  ph_0.025  ph_0.090  ph_0.169