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Element abundances from B stars in the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

A. Jüttner ,
O. Stahl ,
B. Wolf  and
B. Baschek
A. Jüttner
Affiliation:
Landessternwarte Heidelberg, D-6900 Heidelberg, FR Germany
O. Stahl
Affiliation:
Landessternwarte Heidelberg, D-6900 Heidelberg, FR Germany
B. Wolf
Affiliation:
Landessternwarte Heidelberg, D-6900 Heidelberg, FR Germany
B. Baschek
Affiliation:
Institut für Theoretische Astrophysik, D-6900 Heidelberg, FR Germany

Abstract

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High resolution spectrograms of B stars in the blue globular cluster NGC 2004, located in the Large Magellanic Cloud (LMC), have been used to derive chemical abundances, differentially with respect to a galactic comparison star.

Type
Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 388 - 389
Copyright
Copyright © Kluwer 1991 

References

Jüttner, A., Reitermann, A., Stahl, O., Wolf, B. (1989), Astron. Astrophys. Suppl. 81, 93.Google Scholar
Reitermann, A., Baschek, B., Stahl, O., Wolf, B., (1990), Astron. Astrophys. in press.Google Scholar