activity
20222026
most citedA transiting giant planet in orbit around a 0.2-solar-mass host star

10 citations · 25 across the 20 of their papers we have counts for

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Showing 2026Show all

6 papers · 1 filter

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.HE2026

Pulsational mass loss from supermassive stars creates the compact shells of Little Red Dots

Devesh Nandal, Igor Chilingarian, Chris Nagele +3

Little Red Dots (LRDs) have emerged as one of the central puzzles of the JWST era. Their spectra increasingly require dense gas close to the source, yet the physical origin of that…

astro-ph.GA2026

Ram-pressure-induced star formation in low-mass galaxies infalling on-to the Coma cluster: insights from DESI

Kirill A. Grishin, Igor V. Chilingarian, Gary A. Mamon +2

Ram-pressure stripping is a key driver of galaxy morphological transformation in clusters, contributing to the formation of quenched, especially dwarf, populations. Ram-pressure co…

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.IM2026

Website with interactive visualization of multivariate astronomical time series

M. Volkov, M. Demianenko, D. Matveev +2

Light curves represent astronomical time series of flux measured across one or more photometric bands. With the rapid growth of large-scale sky surveys, time-domain astronomy has b…