Some Self-consistent Models of Infinitely thin Stellar Disks with an Elliptical Velocity Distribution

Articles in the same Issue

1. How does the Mass Transport in Disk Galaxy Models Influence the Character of Orbits?
2. Diffusional Separation of Calcium Isotopes in Chemically Peculiar Stellar Atmospheres
3. Improvements in the Spherical Collapse Model and Dark Energy Cosmologies
4. Stochasticity in Star Clusters: Reduced Random Sampling Method
5. Stochastic 2-D Models of Galaxy Disk Evolution. The Galaxy M33
6. Models of Late-type Disk Galaxies: 1-D Versus 2-D
7. Orbits of the Asteroids Discovered at the Molėtai Observatory in 2000–2004
8. Catalogue of Bright IDS Stars with Extensive Cross-Identifications
9. The Half-Century History of Studies of Romano’s Star
10. Observations of Two Unusual Eclipsing Binaries, FN Cam and AG Vir
11. Medium Resolution Spectroscopy and Chemical Composition of Galactic Globular Clusters
12. On the Mass Distribution of Stellar-Mass Black Holes
13. On Cluster Rotation in the Galactic Tidal Field
14. Outer Rings in Early-type Galaxies: From Vorontsov-Velyaminov to Present
15. On the Construction of a New 3D Atlas of Stellar Spectral Energy Distributions
16. Some Self-consistent Models of Infinitely thin Stellar Disks with an Elliptical Velocity Distribution