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

Bibcode
2008PhDT........12F
Fabbian, D.
Bibliographical reference

PhD Thesis, Australian National Univ., 2008

Advertised on:
1
2008
Number of authors
1
IAC number of authors
0
Citations
0
Refereed citations
0
Description
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
Type
Non-refereed

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