Titlebook: Accretion Disks — New Aspects; Proceedings of the E Emmi Meyer-Hofmeister,Henk Spruit Conference proceedings 1997 Springer-Verlag Berlin He

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Gillian Morrison,Joshua M. Tobinnecessarily coplanar with the disc midplane..The calculations are relevant to a number of observed astrophysical phenomena, including the precession of jets associated with young stars, the high spectral index of some T Tauri stars, and the light curves of X-ray binaries such as Hercules X-1 which s

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Jennifer Cone,Demetrios Demetriadesgenerally possess a sub-Keplerian angular momentum distribution and have maximum temperatures in the range 10. – 10. K. Accretion discs around rotating black holes are hotter and deposit less angular momentum on the central object than accretion discs around Schwarzschild black holes.

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Anatomy of the Subaxial Cervical Spineal and short term variability characteristics of the hard X-ray emission were observed in the low spectral state of several black hole binaries. Possible relation of these variations with change of the mass accretion rate and low/high spectral state transitions is discussed.