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Black-Hole Accretion Disks

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Black-Hole Accretion Disks

Towards a New Paradigm



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Black-Hole Accretion Disks by Shoji Kato
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Since publication of the first edition, models of advection-dominated accretion flows and their comparison with observations have been much developed and deepened, including the cases of super-Eddington accretion. The launch of the Rossi X-ray Timing Explorer led to the discovery of high-frequency oscillations, which opened a new field of discoseismology. In addition, development of observational techniques show that the time when we see a direct image or silhouette of black holes is in the near future. Considering these situations, we fully revised the first edition in order to meet the developments mentioned above.
Release date Australia
March 1st, 2008
Trans Pacific Press
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