Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2010-12-02
EAS Publications Series 43 (2010) 199-214
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
16 pages, 13 figures
Scientific paper
10.1051/eas/1043015
Line-formation calculations in the Rayleigh-Jeans tail of the spectral energy distribution are complicated by an amplification of non-LTE effects. For hot stars this can make quantitative modelling of spectral lines in the near-IR challenging. An introduction to the modelling problems is given and several examples in the context of near-IR line formation for hydrogen and helium are discussed.
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