Mitsuru Takeuchi
Abstract
Open-access reader
The new model for X-ray fluctuations of Cyg X-1, which is based on the fluid dynamics, is presented. The model is the optically thin and advection-dominated accretion disk model, which has a critical behavior.
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The new model for X-ray fluctuations of Cyg X-1, which is based on the fluid dynamics, is presented. The model is the optically thin and advection-dominated accretion disk model, which has a critical behavior.
Key concepts: Advection, Accretion (finance), Accretion disc, Physics, Astrophysics, Thin disk, Dynamics (music), Quantum mechanics