Line blanketing by iron group elements in non-LTE model atmospheres of hot stars

Details Line blanketing by iron group elements in non-LTE model atmospheres of hot stars Line blanketing by iron group elements in non-LTE model atmospheres of hot stars

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ssrv...66..147d&link_type=abstract

Space Science Reviews, Volume 66, Issue 1-4, pp. 147-152

Physics

2

Stars, Early-Type, Stars: Atmospheres, Radiative Transfer, Line: Formation, Methods: Numerical, Ultraviolet: Stars

Scientific paper

We report on our recent progress in modeling non-LTE atmospheres of O-stars including blanketing by lines from the iron group elements. The numerical method to account for the huge number of atomic levels and line transitions is presented. Results of exploratory model calculations examining the effects on the temperature structure, the hydrogen and helium line profiles and UV/EUV fluxes are discussed.

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