activity
20192025
most citedThe Influence of the Galactic Bar on the Dynamics of Globular Clusters

8 citations · 16 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025

Counting mass with Gaia: Mass Density of stars and stellar remnants in the solar neighborhood

Artem Lutsenko, Giovanni Carraro, Vladimir Korchagin +2

In the light of new full-sky surveys, many attempts of creating a consistent Galactic model were made. The main interest is to estimate the still poorly understood dark matter cont…

astro-ph.GA2025★ 5 cited

Determining the Scale Length and Height of the Milky Way's Thick Disc Using RR~Lyrae

Roman Tkachenko, Katherine Vieira, Artem Lutsenko +2

Using the RR Lyrae surveys Gaia DR3 Specific Objects Study, PanSTARRS1 and ASAS-SN-II, we determine the Milky Way's thick disc scale length and scale height as well as the radial s…

astro-ph.GA2023★ 2 cited

Resonant Effects of a Bar on the Galactic Disk Kinematics Perpendicular to Its Plane

Vladimir Korchagin, Artem Lutsenko, Roman Tkachenko +2

Detailed analysis of kinematics of the Milky Way disk in the solar neighborhood based on the GAIA DR3 catalog reveals the existence of peculiarities in the stellar velocity distrib…

astro-ph.GA2023★ 8 cited

The Influence of the Galactic Bar on the Dynamics of Globular Clusters

Roman Tkachenko, Vladimir Korchagin, Anna Jmailova +2

We make use of recent estimates for the parameters of the Milky Way's halo globular clusters and study the influence of the galactic bar on the dynamics of these clusters by comput…

astro-ph.GA2023

Gravitational Instability of Gas-Dust Circumnuclear Disks in Galaxies

Roman Tkachenko, Vladimir Korchagin, Boris Jmailov

We numerically study the origin of the multi-armed spiral structure observed in the circumnuclear gaseous mini-disks of nearby galaxies. We show that the presence of dust in such d…

astro-ph.GA2019★ 1 cited

Local metallicity distribution function derived from Galactic large-scale radial iron pattern modelling

Yu. N. Mishurov, R. V. Tkachenko

We develop an approach for fitting the results of modeling of wriggling radial large scale iron pattern along the Galactic disk, derived over young (high massive) Cepheids, with th…