Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phst..133a4009k&link_type=abstract
Physica Scripta, Volume 133, Issue , pp. 014009 (2008).
Physics
2
Scientific paper
I review some of the present achievements and future challenges of non-local thermodynamic equilibrium (NLTE) line-formation calculations for solar-type stars. It is concluded that the full potential of NLTE still remains to be tapped, in particular in view of the current transition from one-dimensional (1D) hydrostatic to 3D hydrodynamic model atmospheres.
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