Astrophysical Disks Collective and Stochastic Phenomena / edited by Aleksey M. Fridman, Mikhail Ya. Marov, Ilya G. Kovalenko.

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Bibliographic Details
Corporate Author: SpringerLink (Online service)
Other Authors: Fridman, Aleksey M. (Editor), Marov, Mikhail Ya (Editor), Kovalenko, Ilya G. (Editor)
Format: eBook
Language:English
Published: Dordrecht : Springer Netherlands : Imprint: Springer, 2006.
Edition:1st ed. 2006.
Series:Astrophysics and Space Science Library, 337
Springer eBook Collection.
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Online Access:Click to view e-book
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Table of Contents:
  • 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.