The UVES spectrum of HR 6000 (HD 144667)
Paper I (Castelli, F., Kurucz, R.L., Hubrig, S. 2009, A&A,508,401)
Paper II (Castelli, F., Kurucz, R.L. 2010, A&A,520,57)
plot of the STIS spectrum
plot of the UVES spectrum
emission lines
unidentified lines before 2009
interstellar lines
Parameters Teff=13450K, logg=4.30; vturb=0.0 km/s, vsini=1.5 km/s
from Stromgren colors and FeI-FeII ionization equilibrium.
ATLAS12 model atmosphere.
Non solar abundances:log(N/Ntot) Solar Diff(star-sun)
He I -2.11 -1.11 -1.00
Li I -6.54 -10.99 +4.45
Be II -9.78 -10.66 +0.88
B II -10.1 -9.34 -0.76
C I -5.52 ± 0.30 -3.61 -1.91 no fit
C II -5.50 -1.89
N I -6.01 ± 0.47 -4.21 -1.80 no fit
N II -5.23 ± 0.04 -4.21 -1.02
O I -3.68 ± 0.4 -3.35 -0.33
Ne I -5.34 -4.11 -1.23
Na I ≤-5.71 -5.83 ≤+0.12
Mg II -5.45 ± 0.09 -4.45 -1.00
Al II -7.80 ± 0.03 -5.61 -2.19
Al III -7.70 -5.61 -2.09
Si II -6.99 ± 0.64 -4.53 -2.46 no fit
Si III -7.60 ± 0.59 -4.53 -3.07 no fit
Si IV -6.65 -4.53 -2.12
P I -5.53 ± 0.08 -6.63 +1.10
P II -4.55 ± 0.10 -6.63 +2.08
P III -4.76 ± 0.14 -6.63 +1.87
S II -6.36 -4.92 -1.44
Cl I ≤-7.74 -6.54 ≤-1.20
Ca II -5.70 ± 0.09 -5.72 -0.02 Ca II infrared triplet, shift +0.14 A
Sc III -10.0 ± 0.28 -8.88 -1.12
Ti II -6.47 ± 0.13 -7.11 +0.64
Ti III -6.37 ± 0.41 -7.11 +0.74
V II -9.23 ± 0.12 -8.15 -1.08
Cr II -6.10 ± 0.25 -6.42 +0.32
Cr III -6.22 ± 0.25 -6.42 +0.20
Mn II -5.29 ± 0.21 -6.62 +1.33
Mn III -5.79 ± 0.36 -6.62 +0.83
Fe I -3.65 ± 0.07 -4.57 +0.92
Fe II -3.65 ± 0.09 -4.57 +0.92
Fe III -3.78 ± 0.14 -4.57 +0.79
Co II ≤-10.12 -7.11 ≤-3.01
Ni II -6.24 -5.84 -0.40
Ni III -6.64 ± 0.14 -5.84 -0.80
Cu II -10.53 -7.86 -2.67
Zn II ≤-8.84 -7.48 ≤-1.36
Ga II -8.85 -9.02 +0.36
Ga III -8.15 -9.02 +0.86
Ge II ≤-10.64 -8.41 ≤-2.23
As II -9.74 -9.74 0.00
Sr II ≤-10.7 -9.21 ≤-1.49
Y II -8.60 -9.83 +1.23
Y III -7.60 -9.83 +2.23
Xe II -5.23
Hg II -8.20 [+2.71] no trrestrial isotopic composition
adopted isotopic composition:
196=0.15%; 198=0.77%; 199=20%; 200=6.9%, 201=5%, 202=10%, 204=57.2%