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20212026
most citedStar formation in outer rings of S0 galaxies. IV. NGC 254 -- a double-ringed S0 with gas counter-rotation

8 citations · 16 across the 13 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2026

CoRGI in MaNGA - II. NGC 5717: cold-gas accretion and disk growth in a BGG

Damir Gasymov, Ivan Yu. Katkov, Eva K. Grebel +6

Large-scale stellar counter-rotation, in which two coplanar stellar components rotate in opposite directions, is usually interpreted as a signature of external gas accretion. Such…

astro-ph.GA2026

Giant Low-Surface Brightness Galaxies in the Global Picture of Galaxy Formation and Evolution

Fedor M. Kolganov, Igor V. Chilingarian, Anna S. Saburova +5

Giant low-surface brightness galaxies (gLSBGs) challenge standard merger-driven galaxy assembly models due to their large, dynamically cold disks, with radii often larger than 100~…

astro-ph.GA2026

Dynamical Modeling of Kinematically Decoupled Galaxies: Structural Components

V. S. Goradzhanov, D. D. Mishurin, O. K. Sil'chenko +1

We present the results of dynamical modeling of two galaxies with inconsistent kinematics -- PGC 35706 and LEDA 2220522 -- using data from the MaNGA integral-field spectroscopic su…

astro-ph.GA2026

HI Observations of Giant Low Surface Brightness Galaxies

Philip Lah, Nikhil Arora, Ivan Yu. Katko +5

Giant low surface brightness galaxies (gLSBs) are galaxies with extremely extended, faint, optical disks over 50 kpc in radius and have high total masses which can reach 10^12 sola…

astro-ph.GA2025★ 1 cited

MUSE Study of Two Giant Low-surface-brightness Galaxies with Compact Satellites

Anna S. Saburova, Damir Gasymov, Ivan S. Gerasimov +7

Giant low-surface-brightness disk galaxies (gLSBGs) are rare objects with disk radii up-to 160 kpc and dynamical masses of an order of up to 10 . Their very exist…

astro-ph.GA2025★ 2 cited

Optical Emission-Line Properties of eROSITA-selected SDSS-V Galaxies

Nadiia G. Pulatova, Evgenii Rubtsov, Igor V. Chilingarian +21

We present and discuss optical emission line properties obtained from the analysis of Sloan Digital Sky Survey (SDSS) spectra for an X-ray selected sample of 3684 galaxies (0.002 <…

astro-ph.GA2025

A group of merging galaxies falling onto Abell 2142

Aashiya Anitha Shaji, Anaëlle Hallé, Damir Gasymov +3

Galaxy clusters produce a very hostile environment to galaxies, whose gas gets stripped by ram-pressure, suffer galaxy interactions and witness quenching of their star formation. C…

astro-ph.GA2025★ 2 cited

Stellar CoRGI in MaNGA: Stellar Counterrotating Galaxies Identified in the MaNGA Survey

Damir Gasymov, Ivan Yu. Katkov, Evgenii V. Rubtsov +8

Stellar counterrotating (CR) galaxies are systems hosting two large-scale stellar components rotating in opposite directions -- a main, preexisting galaxy body with an older stella…

astro-ph.GA2024

Optical spectroscopy of host-galaxies of intermediate mass black holes: evolution of central black holes

V. Goradzhanov, I. Chilingarian, M. Demianenko +6

Intermediate-mass black holes (IMBHs) with masses below () are pivotal in understanding the origin and growth mechanisms of supermassive black holes (SMBHs…

astro-ph.GA2024

A closer look at the extended edge-on low-surface brightness galaxies

Anna S. Saburova, Damir Gasymov, Evgenii V. Rubtsov +13

To understand the origin of extended disks of low-surface brightness (LSB) galaxies, we studied in detail 4 such systems with large disks seen edge-on. Two of them are edge-on gian…

astro-ph.GA2023★ 1 cited

Probing the History of the Galaxy Assembly of the Counter-rotating Disk Galaxy PGC 66551

Ivan Katkov, Damir Gasymov, Alexei Kniazev +4

Stellar counter-rotation in disk galaxies directly relates to the complex phenomenon of the disk mass assembly believed to be driven by external processes, such as accretion and me…

astro-ph.GA2022

Detailed study of galaxies with the stellar counter-rotation phenomenon

Damir Gasymov, Ivan Katkov

The process of galactic disc growing is still not fully understood. In the majority of disk galaxies the gas and stars are located in the same plane and rotate in the same directio…

astro-ph.IM2021

Fast interactive web-based data visualizer of panoramic spectroscopic surveys

Ivan Katkov, Damir Gasymov, Joseph D. Gelfand +7

Panoramic IFU spectroscopy is a core tool of modern observational astronomy and is especially important for galaxy physics. Many massive IFU surveys, such as SDSS MaNGA (10k target…

astro-ph.GA2021★ 8 cited

Star formation in outer rings of S0 galaxies. IV. NGC 254 -- a double-ringed S0 with gas counter-rotation

Ivan Katkov, Alexei Kniazev, Olga Sil'chenko +1

Although S0 galaxies are usually considered "red and dead", they often demonstrate star formation organized into ring structures. We aim to clarify the nature of this phenomenon an…

astro-ph.IM2021★ 2 cited

Non-parametric stellar LOSVD analysis

Damir Gasymov, Ivan Katkov

Ill-posed inverse problems are common in astronomy, and their solutions are unstable with respect to noise in the data. Solutions of such problems are typically found using two cla…