L-galaxies 2020: Spatially resolved cold gas phases, star formation and chemical enrichment in galactic discs
Henriques, Bruno, Yates, Rob, Fu, Jian, Guo, Qi, Kauffmann, Guinevere, Srisawat, Chaichalit, Thomas, Peter and White, Simon
(2020)
L-galaxies 2020: Spatially resolved cold gas phases, star formation and chemical enrichment in galactic discs.
Monthly Notices of the Royal Astronomical Society (MNRAS), 491 (4).
5795–5814.
ISSN 0035-8711
We have updated the Munich galaxy formation model, L-Galaxies, to follow the radial distributions of stars and atomic and molecular gas in galaxy discs. We include an H2-based star-formation law, as well as a detailed chemical-enrichment model with explicit mass-dependent delay times for SN-II, SN-Ia and AGB stars. Information about the star formation, feedback and chemical-enrichment histories of discs is stored in 12 concentric rings. The new model retains the success of its predecessor in reproducing the observed evolution of the galaxy population, in particular, stellar mass functions and passive fractions over the redshift range 0
Item Type | Article |
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Additional information | © 2023 Oxford University Press. This is the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1093/mnras/stz3233 |
Keywords | astro-ph.ga, astro-ph.co |
Date Deposited | 15 May 2025 15:06 |
Last Modified | 31 May 2025 00:37 |
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picture_as_pdf - 2003.05944v1.pdf
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