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Non-LTE radiative transfer for the study of stellar photospheres and chromops...
The stellar abundance analysis frequently relies on the local thermodynamic equilibrium (LTE) assumption for spectral line formation. This assumption is not always... -
Chemical evolution of the Large Magellanic Cloud
Despite decades of intensive observational and theoretical work, we are still far from a complete and clear understanding of the nearby universe, the Milky Way (MW)...
