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期刊论文
Non-uniqueness of transonic solution for accretion onto a Schwarzschild black hole
Astron. Astrophys. 148, 176-178 (1985)，-0001，（）：
Received September 10, 1984; accepted February 12, 1985 Summary. The fact that the adiabatic transonic accretion of rotating matter onto a black hole has non-unique, bimodal, solution was demonstrated previously only in terms of an approximate, Newtonian, model. Here the correct generalrelativistic equations are used to prove the bimodal character of accretion onto a Schwarzschild black hole.
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