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NLTE Abundances from Magellanic Cloud B Stars

Published online by Cambridge University Press:  25 May 2016

Andreas J. Korn
Affiliation:
Landessternwarte Königstuhl, 69117 Heidelberg, Germany
Bernhard Wolf
Affiliation:
Landessternwarte Königstuhl, 69117 Heidelberg, Germany

Abstract

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Nine MC young globular cluster and field stars are analysed using fully line-blanketed LTE ATLAS 9 atmospheres and the DETAIL/SURFACE non-LTE line formation code. CNO mixing seems to occur much earlier than predicted by standard theory.

Type
Part 3. Massive Stars and 30 Doradus
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Azzopardi, M., & Vigneau, J. 1975, A&AS, 19, 271 Google Scholar
Brunet, J.P., et al. 1975, A&AS, 21, 109 Google Scholar
Charbonnel, , et al. 1993, A&AS, 101, 415 Google Scholar
Gummersbach, C.A., et al. 1998, A&A, 338, 881 Google Scholar
Reitermann, A., Baschek, B., Stahl, O., & Wolf, B. 1990, A&A, 234, 109 Google Scholar
Robertson, J.W. 1974, ApJ, 191, 67 CrossRefGoogle Scholar