activity
20242026
collaborators

5 papers

astro-ph.GA2026

Simulations of collision and sloshing in the galaxy group NGC 5098/5096

Richards P. Albuquerque, Gastão B. Lima Neto, Rubens E. G. Machado +2

The study of galaxy groups is essential to understanding the evolutionary history of large-scale structures in the Universe. These dense environments have a significant impact on g…

astro-ph.GA2025

Structure and kinematics of the interacting group NGC 5098/5096

G. B. Lima Neto, H. V. Capelato, F. Durret +1

Most galaxies in the Universe are found in groups, which have various morphologies and dynamical states. Studying how groups evolve is an important step for our understanding in bo…

astro-ph.HE2024

Orbital motion of NGC 6166 (3C 338) and its impact on the jet morphology at kiloparsec scales

A. S. R. Antas, A. Caproni, R. E. G. Machado +2

In the central region of the galaxy cluster Abell 2199 (A2199) resides the cD galaxy NGC 6166, which spatially coincides with the 3C 338 radio source. Lobes, jets, and a more detac…

astro-ph.CO2024

Simulating the arrival of the southern substructure in the galaxy cluster Abell 1758

Rubens E. G. Machado, Ricardo C. Volert, Richards P. Albuquerque +2

Abell 1758 (z~0.278) is a galaxy cluster composed of two structures: A1758N and A1758S, separated by ~2.2 Mpc. The northern cluster is itself a dissociative merging cluster that ha…

astro-ph.GA2024

Unraveling the collision scenario of the dissociative galaxy cluster Abell 56 through hydrodynamic simulations

Richards P. Albuquerque, Rubens E. G. Machado, Rogério Monteiro-Oliveira

In galaxy cluster collisions, the gas can be separated from dark matter halos. Abell~56 displays signatures of a dissociative bullet-like merger with a possible high inclination an…