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QPO as the RosettaStone forunderstanding blackhole accretion M. A. Abramowicz2005 год

QPO as the Rosetta Stone for understanding black hole accretion
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Аннотация: Abstract Quasi‐periodic oscillations (QPO) seen in the X‐ray fluxes of individual neutron stars and black hole sources are one of most intriguing phenomena in today's astrophysics. The QPO nature is visibly determined by super‐strong Einstein's gravity. I argue here that it also profoundly depends on the MRI turbulence in accretion flows. Understanding the QPO physics may therefore guide accretion theory out of its present state of confusion. Readers will find here an up‐to‐date, comprehensible account of what is known, and what is not, about the QPO physics. (© 2005 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
Год издания: 2005
Авторы: M. A. Abramowicz
Издательство: Wiley
Источник: Astronomische Nachrichten
Ключевые слова: Astrophysical Phenomena and Observations, High-pressure geophysics and materials, Pulsars and Gravitational Waves Research
Другие ссылки: Astronomische Nachrichten (HTML)
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