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Astrophysics and Space Science, Vol. 346, Iss. 1, 2013-07 ,pp. : 127-130

Springer Publishing Company

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A fully relativistic twisted disc around a slowly rotating Kerr black hole: derivation of dynamical equations and the shape of stationary configurations

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Quasinormal modes and Hawking radiation of a Reissner-Nordström black hole surrounded by quintessence

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The need for hypercritical accretion in massive black hole binaries with large Kerr parameters

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