A Quasi-Stationary Twisted Disk Formed as a Result of a Tidal Disruption Event

Articles in the same Issue

1. Phase-Space Model of a Collisionless Stellar Cylinder Embedded in a Rotating Halo
2. Symbolic Dynamics, Mixing and Entropy in the Three-Body Problem
3. Estimating the Vertical Disk Scale Height Using Young Galactic Objects
4. Kernel Density Estimation in the Study of Star Clusters
5. Photometric Study of the Seyfert Galaxy NGC 4151
6. Ejection of Stars with Relativistic Velocities
7. Swing Amplification and Global Modes Reciprocity in Models with Cusps
8. Gravity-Antigravity Interplay in the Local Galaxy Flows
9. Spectroscopic Studies of Early-type Stars with the Kourovka 1.2-m Telescope
10. A Quasi-Stationary Twisted Disk Formed as a Result of a Tidal Disruption Event
11. Orbits of Wide Binaries – New Possibilities
12. Details of the Classification of Symbiotic Stars: The Case of the Symbiotic Nova AG Peg
13. Molecular Clouds and Star Formation Rate in Disk Galaxies
14. Outer Rings in Early-Type Disk Galaxies: Star Formation Rate
15. The Tidal Potential of a Homogeneous Torus with an Elliptical Section of the Sleeve