C1 non-LTE spectral line formation in late-type stars
We present non-Local Thermodynamic Equilibrium (non-LTE) calculations for neutral carbon spectral line formation, carried out for a grid of model atmospheres covering the range of late-type stars. The results of our detailed calculations suggest that the
|Collections||ANU Research Publications|
|Book Title:||From Lithium to Uranium (S228)|
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