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20132022
most citedA multi-wavelength study of spiral structure in galaxies. I. General characteristics in the optical

43 citations · 134 across the 8 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA202115 cited

Fractal dimension of optical cirrus in Stripe82

Alexander A. Marchuk, Anton A. Smirnov, Aleksandr V. Mosenkov +4

The geometric characteristics of dust clouds provide important information on the physical processes that structure such clouds. One of such characteristics is the fractal dim…

astro-ph.GA202115 cited

Isochrone fitting of Galactic globular clusters -- III. NGC\,288, NGC\,362, and NGC\,6218 (M12)

George A. Gontcharov, Maxim Yu. Khovritchev, Aleksandr V. Mosenkov +6

We present new isochrone fits to colour-magnitude diagrams of the Galactic globular clusters NGC\,288, NGC\,362, and NGC\,6218 (M12). We utilize a lot of photometric bands from the…

astro-ph.GA2020

Investigation of the parameters of spiral pattern in galaxies: the arm width

Aleksandr Mosenkov, Sergey Savchenko, Alexander Marchuk

In this work we determine the parameters of spiral structure for a sample of face-on spiral galaxies. In practice, the solution of this problem is a hard task because of the divers…

astro-ph.GA202043 cited

A multi-wavelength study of spiral structure in galaxies. I. General characteristics in the optical

Sergey Savchenko, Alexander Marchuk, Aleksandr Mosenkov +1

Different spiral generation mechanisms are expected to produce different morphological and kinematic features. In this first paper in a series we carefully study the parameters of…

astro-ph.GA2018

Gravitational instability and star formation in NGC 628

A. A. Marchuk

The gas-stars instability criterion for infinitesimally thin disc was applied to the galaxy NGC 628. Instead of using the azimuthally averaged profiles of data the maps of the gas…

astro-ph.GA201711 cited

Reconstructing the velocity dispersion profiles from the line-of-sight kinematic data in disc galaxies

A. A. Marchuk, N. Y. Sotnikova

We present a modification of the method for reconstructing the stellar velocity ellipsoid (SVE) in disc galaxies. Our version does not need any parametrization of the velocity disp…