On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy

A. O. Gromov; I. I. Nikiforov; L. P. Ossipkov

doi:10.1515/astro-2017-0214

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On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy

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Published/Copyright: February 18, 2017

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From the journal Open Astronomy Volume 24 Issue 2

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Gromov, A. O., Nikiforov, I. I. and Ossipkov, L. P.. "On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy" Open Astronomy, vol. 24, no. 2, 2015, pp. 150-156. https://doi.org/10.1515/astro-2017-0214

Gromov, A., Nikiforov, I. & Ossipkov, L. (2015). On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy. Open Astronomy, 24(2), 150-156. https://doi.org/10.1515/astro-2017-0214

Gromov, A., Nikiforov, I. and Ossipkov, L. (2015) On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy. Open Astronomy, Vol. 24 (Issue 2), pp. 150-156. https://doi.org/10.1515/astro-2017-0214

Gromov, A. O., Nikiforov, I. I. and Ossipkov, L. P.. "On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy" Open Astronomy 24, no. 2 (2015): 150-156. https://doi.org/10.1515/astro-2017-0214

Gromov A, Nikiforov I, Ossipkov L. On the Possibility of Applying the Quasi-Isothermal Stäckel’s Model to Our Galaxy. Open Astronomy. 2015;24(2): 150-156. https://doi.org/10.1515/astro-2017-0214

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Received: 2015-3-25

Accepted: 2015-4-20

Published Online: 2017-2-18

Published in Print: 2015-6-1

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Keywords for this article

methods: analytical; Galaxy: kinematics and dynamics

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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