Abstract
Model atmosphere analyses have been done for the two brightest stars of the Magellanic Clouds: HD 33579 in the Large Magellanic Cloud and HD 7583 in the Small Magellanic Cloud. The results are presented and discussed in connection with the chemical evolution of the Galaxy.
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© 1974 Springer-Verlag, Berlin, Heidelberg
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Wolf, B. (1974). Fine Analytic Abundance Determination of Magellanic Cloud A-Supergiants and its Importance for the Discrimination of Theories for the Chemical Evolution of the Galaxy. In: Mavridis, L.N. (eds) Proceedings of the First European Astronomical Meeting Athens, September 4–9, 1972. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-65666-8_23
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DOI: https://doi.org/10.1007/978-3-642-65666-8_23
Publisher Name: Springer, Berlin, Heidelberg
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