Astrophysical disks : collective and stochastic phenomena
著者
書誌事項
Astrophysical disks : collective and stochastic phenomena
（Astrophysics and space science library, v. 337）
Springer, c2006
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注記
Includes bibliographical references and index
内容説明・目次
内容説明
This book deals with collective and stochastic processes in astrophysical disks involving theory, observations, and the results of modelling. It examines the spiral-vortex structure in galactic and accretion disks, and stochastic and ordered structures in developed turbulence. The book advances the study in this important branch of astrophysics and will benefit professional researchers, lecturers, and graduate students.
目次
Invited Papers.- The Over-Reflection Instability: Myth or Reality?.- Chaotic and Ordered Structures in the Developed Turbulence.- Internal Structure of Thin Accretion Disks.- Disc Formation in Binary be Stars.- Accretion Disks Around Black Holes with Account of Magnetic Fields.- Supercritical Accretion Disk in SS433.- Galactic Vortices.- Spiral Perturbations in Disk Galaxies Observed in NIR.- The Role of Ordered and Chaotic Motion in N-Body Models of Elliptical Galaxies Models.- Oral Contributions.- Gamma-Ray Burst Interaction with Dense Interstellar Medium.- Morphology of the Interaction between the Stream and Cool Accretion Disc in Semidetached Binaries.- Computer Modeling of Non-Stationary Gas Quasi-Keplerian Disk.- 3D Structure of Gaseous Disks in Spiral Galaxies.- Hydrodynamical Turbulence in Accretion Discs.- 2D-Simulations of Subcritical and Supercritical Accretion Disks Around Black Holes.- Separate Circumnuclear Stellar and Gaseous Disks in Disk Galaxies.- Bending Instability Galaxies: The Stellar Disk Thickness and the Mass of Spheroidal Component.- Disk-to-halo Mass Ratio Evaluations Based on the Numerical Models of Collisionless Disks.- Posters.- Global Irregularities of Spiral Patterns in Galaxies: Manifestation of hydrodynamic Instabilities?.- The Morphology of Gaseous Flows in Z and in the Active State.- Self-Consistent Gas and Stellar Dynamics of Disk Galaxies: A Problem of Dark Mass.- Numerical Simulation of Expanding Shock Waves in the Young Stars Objects.
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