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...
Συγγραφή απο Οργανισμό/Αρχή: | |
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Άλλοι συγγραφείς: | , , |
Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
Γλώσσα: | English |
Έκδοση: |
Dordrecht :
Springer Netherlands,
2006.
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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.