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astro-ph.GA2026

Resolved Dust-Gas-Metallicity relations in nearby spiral galaxies

Vidhi Tailor, Viviana Casasola, Francesco Calura +17

Context: Understanding the interstellar medium (ISM) requires high-resolution, multi-component mapping to capture its complex physical structure. Nearby spiral galaxies, with their…

astro-ph.GA2026

Determining Total Infrared Luminosities from Submm Measurements of High Redshift Galaxies

Maria Emilia De Rossi, George H. Rieke, Christina C. Williams +6

Determining total infrared luminosities for very high redshift galaxies is important to estimate the rate of star formation in heavily dust-embedded environments. It is also challe…

astro-ph.GA2026

Characterizing the Formation and Evolution of S0-galaxies (CaFES-0): Their formation pathways around Galaxy Clusters

Diego Pallero, Yara L. Jaffé, Amelia Fraser-McKelvie +7

The formation pathways of lenticular galaxies (S0s), which lie morphologically between elliptical and spiral galaxies, remain a topic of active research. Environmental effects, mer…

astro-ph.GA2026

The S-PLUS Fornax Project (S+FP): Fornax-like clusters in cosmological hydrodynamical simulations

L. J. Zenocratti, A. V. Smith Castelli, M. E. De Rossi +12

The Fornax galaxy cluster constitutes a suitable laboratory to explore the evolution of galaxies in a dense environment. Recently, the Southern Photometric Local Universe Survey (S…

astro-ph.GA2026

Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31

Salvador E. Grimozzi, Maria Emilia De Rossi, Andreea S. Font

We investigate the origin of the scatter in supermassive black hole (BH) masses among L* galaxies, using the ARTEMIS and EAGLE simulations. We classify galaxies by their central BH…

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…