Effects of line-blocking on the non-LTE Fe I spectral line formation.
The effects of background line opacity (line-blocking) in statistical equilibrium calculations for Fe in late-type stellar atmospheres have been investigated using an extensive and up-to-date model atom with radiative data primarily from the IRON Project. The background metal line opacities have been computed using data from the MARCS stellar model atmospheres. While accounting for this line opacity is important at solar metallicity, the differences between calculations including and excluding...[Show more]
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
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