Chemical compositions of stars in the light of non-LTE spectral line formation: the evolution of carbon and oxygen in the Galaxy

Details Chemical compositions of stars in the light of non-LTE spectral line formation: the evolution of carbon and oxygen in the Galaxy Chemical compositions of stars in the light of non-LTE spectral line formation: the evolution of carbon and oxygen in the Galaxy

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phdt........12f&link_type=abstract

PhD Thesis, Australian National Univ., 2008

Physics

Line: Formation, Stars: Abundances, Stars: Late-Type, Galaxy: Abundances, Galaxy: Evolution

Scientific paper

Non-LTE effects affect the formation of many spectral features in the spectra of late-type stars. This thesis investigates the effect on carbon and oxygen abundances. The non-LTE calculations have been performed with the code MULTI, using MARCS atmospheric models with 4500

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