activity
20242026
most citedThe role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies

8 citations · 10 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

The properties of central stellar knots embedded in galactic bulges of CIELO simulations

Belén Acosta-Tripailao, Patricia B. Tissera, Manuela Zoccali +7

Deeply bound stellar substructures of about 1 kpc at the center of bulges are found in a subset of galaxies from the cosmological chemo-hydrodynamical zoom-in CIELO simulation suit…

astro-ph.GA2026

Angular momentum evolution in the CIELO simulations. I. Temporal evolution of gas-stellar misalignments and baryonic merger timing

Catalina Casanueva-Villarreal, Patricia B. Tissera, Nelson Padilla +4

Gas-stellar kinematic misalignments trace how galaxies assemble and reorient their angular momentum. Although well documented locally, their continuous evolution remains largely un…

astro-ph.GA2025

The heartbeat of stellar halos: Insights from the stellar halo mass-metallicity relation

Jenny Gonzalez-Jara, Patricia B. Tissera, Antonela Monachesi +5

This work investigates the presence and evolution of the MZhR from redshift z=3.5 to z=0, and identifies when galaxies settle on the present-day MZhR. We used central galaxies with…

astro-ph.CO2025

Aletheia: Emulating the non-linear matter power spectrum in the context of evolution mapping

Ariel G. Sanchez, Andrés N. Ruiz, Facundo Rodriguez +7

We present Aletheia, a new emulator of the non-linear matter power spectrum, , built upon the evolution mapping framework. This framework addresses the limitations of traditi…

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★ 1 cited

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.GA2025★ 1 cited

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

The CIELO Project: The Chemo-dynamical properties of gaLaxies and the cosmic web

Patricia Tissera, Lucas Bignone, Jenny Gonzalez-Jara +13

The CIELO project introduces a novel set of chemo-dynamical zoom-in simulations designed to simultaneously resolve galaxies and their nearby environments. The initial conditions in…

astro-ph.GA2024

Unveiling the formation channels of stellar halos through their chemical fingerprints

Jenny Gonzalez-Jara, Patricia B. Tissera, Antonela Monachesi +6

Stellar halos around galaxies contain key information about their formation and assembly history. Using simulations, we can trace the origins of different stellar populations in th…

astro-ph.GA2024★ 8 cited

The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies

Elisa A. Tau, Antonela Monachesi, Facundo A. Gomez +7

The stellar halos of dwarf galaxies are becoming an object of interest in the extragalactic community due to their detection in some recent observations. Additionally, new cosmolog…