Fe I lines in the spectra of cool stars: NLTE corrections of iron abundance in the Sun.

Details Fe I lines in the spectra of cool stars: NLTE corrections of iron abundance in the Sun. Fe I lines in the spectra of cool stars: NLTE corrections of iron abundance in the Sun.

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999kfnt...15..523s&link_type=abstract

Kinematika Fiz. Nebesn. Tel, Tom 15, No. 6, p. 523 - 535

Physics

1

Iron Lines: Cool Stars, Iron Lines: Solar Photosphere, Iron Lines: Stellar Atmospheres

Scientific paper

A self-consistent solution of the kinetic and radiative transfer equations is carried out for two types of solar-like model atmospheres using a very realistic iron atomic model. The results were used to investigate the NLTE effects in the solar photospheric iron abundance determined from Fe I lines. The author shows that the errors in the solar photospheric abundance due to these effects can be statistically described by functions depending on line formation height and excitation potential of the lower level.

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