References
See,e.g.,Giacconi:Binary X-raysources, invited talk delivered at theSolvay Meeting, Bruxelles, 1973, to appear in theProceedings.
See,e. g. R. Ruffini:Neutron stars and black holes in our galaxy, invited talk delivered at theSolvay Meeting, Bruxelles, 1973, to appear in theProceedings.
For a lucid and detailed treatment of plasma accreting in the magnetic field of a normal star see the classical work ofM. N. Mestel:Roy. Amer. Soc.,119, 223 (1959). Accretion of plasma into a black hole has recently been examined byR. Ruffini andJ. Wilson: to be published.
For the analysis of the electromagnetic structure of the field of a black hole seeD. Christodoulou andR. Ruffini:On the electrodynamics of collapsed objects, inBlack Holes, edited byB. DeWitt andC. DeWitt (New York, N. Y., 1973).
Here and in the following we are using geometrized unitsG=c=1.
D. Christodoulou: private communication to one of us (R.R.).
E. T. Newman, E. Couch, R. Chinnapared, A. Exton, A. Prakash andR. Torrence:Journ. Math. Phys.,6, 918 (1965).
F. Hoyle:Communication at the 1971 Meeting on Collapsed Objects in Honour of the 60th Birthday of W. Fowler, Cambridge, England.
R. Ruffini andJ. R. Wilson: to be published.
R. Leach: Senior Thesis, presented at Princeton University, unpublished (1974).
See,e.g.,M. Abramowitz andI. A. Stegun:Handbook of Mathematical Functions (1970).
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Work partially supported by N.S.F. Grant GP 30799X to Princeton University.
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Hanni, R.S., Ruffini, R. Schwarzschild black hole in an asymptotically uniform magnetic field. Lett. Nuovo Cimento 15, 189–194 (1976). https://doi.org/10.1007/BF02727480
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DOI: https://doi.org/10.1007/BF02727480