Astrophysical disks Collective and Stochastic Phenomena /

The book deals with collective and stochastic processes in astrophysical discs involving theory, observations, and the results of modelling. Among others, it examines the spiral-vortex structure in galactic and accretion disks , stochastic and ordered structures in the developed turbulence. It also...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Συγγραφή απο Οργανισμό/Αρχή: SpringerLink (Online service)
Άλλοι συγγραφείς: Fridman, Alexei M. (Επιμελητής έκδοσης), Marov, Mikhail Ya (Επιμελητής έκδοσης), Kovalenko, Ilya G. (Επιμελητής έκδοσης)
Μορφή: Ηλεκτρονική πηγή Ηλ. βιβλίο
Γλώσσα:English
Έκδοση: Dordrecht : Springer Netherlands, 2006.
Θέματα:
Διαθέσιμο Online:Full Text via HEAL-Link
Πίνακας περιεχομένων:
  • 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.