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Astron. Astrophys. 334, 210-220 (1998)

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Acknowledgements

We are grateful to S.E. Woosley and S.P. Owocki for helpful discussions, to J. Fliegner for providing us with an implementation of rotational physics in the stellar evolution code, and to A. Weiss for supplying us with his recent opacity tables. This work has been supported by the Deutsche Forschungsgemeinschaft through grant No. La 587/15-1.

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© European Southern Observatory (ESO) 1998

Online publication: May 12, 1998

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