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Astrophysical Disks
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Astrophysical Disks Collective and Stochastic Phenomena / edited by Aleksey M. Fridman, Mikhail Ya. Marov, Ilya G. Kovalenko.
Saved in:
书目详细资料
企业作者:
SpringerLink (Online service)
其他作者:
Fridman, Aleksey M.
(Editor)
,
Marov, Mikhail Ya
(Editor)
,
Kovalenko, Ilya G.
(Editor)
格式:
电子书
语言:
English
出版:
Dordrecht :
Springer Netherlands : Imprint: Springer,
2006.
版:
1st ed. 2006.
丛编:
Astrophysics and Space Science Library,
337
Springer eBook Collection.
主题:
Astrophysics.
Observations, Astronomical.
Astronomy—Observations.
Computers.
Mathematical models.
Physics.
Statistical physics.
Dynamical systems.
Electronic resources (E-books)
在线阅读:
Click to view e-book
Holy Cross Note:
Loaded electronically.
Electronic access restricted to members of the Holy Cross Community.
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书本目录
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书本目录:
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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