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Astron. Astrophys. 319, 1025-1035 (1997)

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Acknowledgements

This work was supported by Swedish Natural Science Research Foundation (NFR). I thank M. Camenzind and M. Haehnelt for ideas the numerical calculations in this paper took advantage from and R. Khanna for helpful discussions. F. Quist is acknowledged for reading the manuscript. I am grateful to the referee, I. Okamoto, for clarifying comments, and especially for suggesting an estimate of the energy and angular momentum losses of the black hole from the current distribution.

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© European Southern Observatory (ESO) 1997

Online publication: July 3, 1998
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