activity
20242026
collaborators

9 papers

astro-ph.GA2026

Reconstructing chemical enrichment pathways in disc galaxies: A phylogenetic approach

Brian Tapia-Contreras, Patricia B. Tissera, Emanuel Sillero +11

Phylogenetic methods, traditionally used in biology to trace the evolutionary relationships among species, are emerging as a powerful framework to reconstruct evolutionary processe…

astro-ph.GA2026

Metal-loaded outflows in sub-Milky Way galaxies in the CIELO simulations

Valentina P. Miranda, Patricia B. Tissera, Emanuel Sillero +5

Supernova (SN) feedback-driven galactic outflows are a key physical process that contributes to the baryon cycle by regulating the star formation activity, reducing the amount of m…

astro-ph.GA2026

Aligned and misaligned metallicity gradients in young stars and star-forming regions in the EAGLE discs

Isha Shailesh, Patricia B. Tissera, Emanuel Sillero

Disc galaxies exhibit radial metallicity gradients in both their stellar and gaseous components. The star-forming gas (SFG) in HII regions and young stars (YSs) trace the recent ev…

astro-ph.GA2025

The mass-metallicity relation of bulges

Ignacio Muñoz-Escobar, Patricia B. Tissera, Jenny Gonzalez-Jara +4

Context. Bulges, located at the central regions of galaxies, are complex structures, expected to be shaped by the physical processes involved in the assembly history of their host…

astro-ph.GA2025

Insight into the physical processes that shape the metallicity profiles in galaxies

Brian Tapia-Contreras, Patricia B. Tissera, Emanuel Sillero +6

The distribution of chemical elements in the star-forming regions can store information on the chemical enrichment history of the galaxies. Negative metallicity gradients are expec…

astro-ph.GA2025

Mocking IFU observations and metallicity diagnostics from cosmological simulations

A. Cornejo-Cárdenas, E. Sillero, P. B. Tissera +4

Hydrodynamic simulations are powerful tools for studying galaxy formation. However, it is crucial to test and improve the sub-grid physics underlying these simulations by comparing…