Cosmological gas accretion of Milky Way-type galaxies and the build-up of galactic discs

Fuente: arXiv
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Autores principales: Nuza, Sebastián E., Scannapieco, Cecilia
Formato: Preprint
Publicado: 2025
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author Nuza, Sebastián E.
Scannapieco, Cecilia
author_facet Nuza, Sebastián E.
Scannapieco, Cecilia
contents In this work, we present results on the assembly of stellar discs belonging to Milky Way-type galaxies in the Auriga simulated sample. We study the net accretion of gas onto the disc region as a function of time and radius to assess the feasibility of the so-called inside-out formation of galaxy discs. We found that most of the galaxies in our sample exhibit an inside-out disc growth, with younger stellar populations preferentially formed in the outer regions as accreted material turns into starts. This produces stable discs as long as late-time accretion is free from significant external perturbations.
format Preprint
id arxiv_https___arxiv_org_abs_2504_02616
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Cosmological gas accretion of Milky Way-type galaxies and the build-up of galactic discs
Nuza, Sebastián E.
Scannapieco, Cecilia
Astrophysics of Galaxies
In this work, we present results on the assembly of stellar discs belonging to Milky Way-type galaxies in the Auriga simulated sample. We study the net accretion of gas onto the disc region as a function of time and radius to assess the feasibility of the so-called inside-out formation of galaxy discs. We found that most of the galaxies in our sample exhibit an inside-out disc growth, with younger stellar populations preferentially formed in the outer regions as accreted material turns into starts. This produces stable discs as long as late-time accretion is free from significant external perturbations.
title Cosmological gas accretion of Milky Way-type galaxies and the build-up of galactic discs
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2504.02616