Article
Open Access
The Evolution of a Supermassive Retrograde Binary Embedded in an Accretion Disk
-
P. B. Ivanov
,
J. C. B. Papaloizou
Published/Copyright:
February 18, 2017
Received: 2015-3-25
Accepted: 2015-4-20
Published Online: 2017-2-18
Published in Print: 2015-6-1
© 2015 P. B. Ivanov et al., published by De Gruyter Open
Articles in the same Issue
- Galactic Spiral Pattern beyond the Optical Size Induced by the Triaxial Dark Halo
- High Resolution Gravitational Lens Model
- Detection of Unresolved Binaries with Multicolor Photometry
- On the Formation of Tails in the Galactic Tidal Field
- On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy
- Visual Binaries: Cross-Matching and Compiling of a Comprehensive List
- The Evolution of a Supermassive Retrograde Binary Embedded in an Accretion Disk
- On Equilibrium Figures of Particle Clouds around the Sun and Stars
- BSDB: A New Consistent Designation Scheme for Identifying Objects in Binary and Multiple Stars
- Star Formation and Galaxy Dynamo Equations with Random Coefficients
- Destruction of Globular Clusters in the Galactic Gravitational Field
- Stochasticity of Galactic Orbits of Star Clusters
- Velocity Dispersion of Ionized Gas and Multiple Supernova Explosions
Keywords for this article
accretion disks;
binaries;
hydrodynamics;
galaxies: quasars: supermassive black holes;
planet-disk interactions
Creative Commons
BY-NC-ND 3.0
Articles in the same Issue
- Galactic Spiral Pattern beyond the Optical Size Induced by the Triaxial Dark Halo
- High Resolution Gravitational Lens Model
- Detection of Unresolved Binaries with Multicolor Photometry
- On the Formation of Tails in the Galactic Tidal Field
- On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy
- Visual Binaries: Cross-Matching and Compiling of a Comprehensive List
- The Evolution of a Supermassive Retrograde Binary Embedded in an Accretion Disk
- On Equilibrium Figures of Particle Clouds around the Sun and Stars
- BSDB: A New Consistent Designation Scheme for Identifying Objects in Binary and Multiple Stars
- Star Formation and Galaxy Dynamo Equations with Random Coefficients
- Destruction of Globular Clusters in the Galactic Gravitational Field
- Stochasticity of Galactic Orbits of Star Clusters
- Velocity Dispersion of Ionized Gas and Multiple Supernova Explosions
