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)
Parameters: Teff=7700 K, log g=4.2 from Ryabchikova et al., A&A 322, 234, (1997)
vsini=16 km/sec from our CRIRES spectra; R=95000
OBSERVED spectra are shifted by +44 km/sec in order to be overimposed on
synthetic spectra with Ritz wavelengths.
STELLAR ABUNDANCES used to compute the synthetic spectrum:
Those for O, Na, and P are upper limits, because lines were predicted but
were not observed for these elements.
The abundances of the not listed elements are solar.
star sun
C -4.00 -3.52
O -3.71 -3.21
Na -6.00 -5.71
Mg -4.46 -4.46
Al -5.10 -5.57
Si -3.90 -4.49
P -7.80 -6.59
Ca -5.08 -5.68
Cr -5.37 -6.37
Fe -4.35 -4.54
Sr -7.10 -9.07
Ce -5.10 -10.46
identified lines
