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Astron. Astrophys. 343, 325-332 (1999)

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References

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Note added in proof: Very recently, Lovås (1998) compared the pseudo-potentials of Paczynski & Wiita (1980), of Nowak & Wagoner (1991) and of Artemova et al. (1996) with the exact black hole fields. For each of the cases, she computed several quantities crucial in the theory of (optically thin) accretion discs and proposed to use [FORMULA] for non-rotating holes while the potentials by Artemova et al. for rotating holes.

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© European Southern Observatory (ESO) 1999

Online publication: March 1, 1999
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