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20232026
most citedGalaxies decomposition with spiral arms -- II: A multiwavelength case study of M 51

15 citations · 38 across the 15 of their papers we have counts for

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15 papers · 1 filter

astro-ph.GA2026

The Edge-on Galaxies in the DESI survey (EGIDE): sample building and photometry

Alexander A. Marchuk, Sergey S. Savchenko, Dmitry I. Makarov +7

We present the EGIDE (The Edge-on Galaxies in the DESI survey) project - a catalogue of 149,215 edge-on galaxy candidates created using the data of the DESI Legacy Imaging Survey D…

astro-ph.GA2026

Projection-Enhanced Disk Breaks: Evidence from Deep Photometric Decomposition

Sergey S. Savchenko, Ilia V. Chugunov, Alexander A. Marchuk +5

Radial brightness profiles of disk galaxies often exhibit so-called breaks -- locations where their exponential-scale length abruptly changes. Some galaxies have downbending (Type…

astro-ph.GA2026

A New Cartwheel-like Collisional Ring Galaxy

Vladimir P. Reshetnikov, Sergey S. Savchenko, Alexander A. Marchuk +5

We report the discovery of a new Cartwheel-type collisional ring galaxy, PGC\,1112751, which we named ``Eridanus Wheel'' (EW). Such systems result from head-on collisions between g…

astro-ph.GA2026

Clumps in spiral galaxies at : Disentangling two spatial modes of star formation

Ilia V. Chugunov, Alexander A. Marchuk

At high redshifts, star formation in galaxies is more often concentrated in clumps than in spiral arms. Although clumps are actively studied, it is rarely done considering spiral a…

astro-ph.GA2026

Galactic disc warps from to modern epoch: ruling out observational effects

Ilia V. Chugunov, Vladimir P. Reshetnikov, Alexander A. Marchuk

A significant fraction of galaxies show warps in their discs, usually noticeable at its periphery. The exact origin of this phenomenon is not fully established, although multiple w…

astro-ph.GA2025★ 9 cited

Galactic warps: from cosmic noon to the current epoch

Vladimir P. Reshetnikov, Ilia V. Chugunov, Alexander A. Marchuk +6

Approximately half of all disc galaxies exhibit appreciable warps in both their stellar and HI discs. The typical warp amplitude is small (a few degrees), and only becomes noticeab…