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Astron. Astrophys. 317, 140-163 (1997)

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Acknowledgements

The post-collapse models provided to us by S.W. Bruenn and W. Hillebrandt to be used as initial models in our simulations are kindly acknowledged. We would like to thank Maximilian Ruffert, Gerhard Schäfer, and Thomas Zwerger for many enlightening discussions and valuable comments. In particular, we are grateful to Thomas Zwerger for providing to us his 3D Poisson solver. All hydrodynamical simulations were performed on the CRAY-YMP 4/64 of the Rechenzentrum Garching. The Rechenzentrum Garching is also acknowledged for generous financial support concerning the publication costs.

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© European Southern Observatory (ESO) 1997

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