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most citedGlobular clusters in the central region of the Milky Way galaxy I. Bar influence on the orbit parameters according to Gaia EDR3

3 citations · 5 across the 10 of their papers we have counts for

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astro-ph.GA2025

Analysis of Orbital Dynamics of Globular Clusters in the Central Region of the Milky Way

A. T. Bajkova, A. A. Smirnov, V. V. Bobylev

The regularity/chaoticity of orbits of 45 globular clusters in the central region of the Galaxy with a radius of 3.5 kpc, which are subject to the greatest influence of the elongat…

astro-ph.GA2025

Relationship between Poincaré Sections and Spectral Characteristics of Orbits of Globular Clusters in the Central Region of the Galaxy

Anisa Bajkova, Anton Smirnov, Vadim Bobylev

In the paper, orbital dynamics, regular or chaotic, of globular clusters (GCs) in the central region of the Galaxy, which is subject to the greatest influence of the rotating bar,…

astro-ph.GA2025

Variations of angular momentum as an indicator of orbital chaos of globular clusters in the central region of the Galaxy with a bar

A. T. ~Bajkova, A. A. ~Smirnov, V. V. ~Bobylev

It is shown how the violation of the invariance of the -component of the orbital angular momentum in the axially symmetric potential of the Galaxy with a bar can serve as…

astro-ph.GA2025★ 1 cited

The Spiral Pattern Speed in the Milky Way Galaxy

Vadim V. Bobylev, Anisa T. Bajkova, Anton A. Smirnov

For a sample of masers, the basic kinematic equations were solved by including the Galactic rotation parameters and the peculiar velocity of the Sun as the unknown variables. Based…

astro-ph.GA2025

Spectral Analysis of the Orbital Dynamics of Globular Clusters in the Central Region of the Milky Way

Anisa Bajkova, Anton Smirnov, Vadim Bobylev

A new method for determining the nature of the orbital motion (chaotic or regular) of globular clusters in the central region of the Galaxy with a radius of 3.5 kpc, which are most…