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astro-ph.GA2025

Formation and evolution of boxy/peanut bulges in the Auriga cosmological simulations

Paula D. López, Francesca Fragkoudi, Sofía A. Cora +5

Boxy/peanut (b/p) or X-shaped bulges have been extensively explored with theory and numerical simulations of isolated galaxies. However, it is only recently that advances in hydrod…

astro-ph.GA2025

The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations

Jonathan S. Gómez, Tomas Hough, Alejandro Jiménez Muñoz +3

Next-generation photometric and spectroscopic surveys will detect faint galaxies in massive clusters, advancing our understanding of galaxy formation in dense environments. Compari…

astro-ph.GA2025

Improving the accuracy of observable distributions for galaxies classified in the Projected Phase Space Diagram

Héctor J. Martínez, Martín de los Rios, Valeria Coenda +4

Studies of galaxy populations classified according to their kinematic behaviours and dynamical state using the Projected Phase Space Diagram (PPSD) are affected by misclassificatio…

astro-ph.GA2025

The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity

Daniela Palma, Ivan Lacerna, M. Celeste Artale +7

We investigated the population of low-mass central galaxies with Mstar = Msun/h, inhabiting regions near massive groups and clusters of galaxies using the TNG300…

astro-ph.GA2024

Connection between feedback processes and the effective yields of EAGLE galaxies

M. C. Zerbo, M. E. De Rossi, M. A. Lara-López +2

The feedback mechanisms triggered by supernova (SN) events and active galactic nuclei (AGN) play a central role in regulating the star formation and shaping galaxy properties. Howe…

astro-ph.GA2024

Unveiling the origins of galactic bars: insights from barred and unbarred galaxies

Paula D. López, Cecilia Scannapieco, Sofía A. Cora +1

A significant fraction of local galaxies exhibit stellar bars, non-axisymmetric structures composed of stars, gas, and dust. Identifying key differences between the properties of b…