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dc.contributor.author
Poulhazan, Pierre Antoine  
dc.contributor.author
Scannapieco, Cecilia  
dc.contributor.author
Creasey, Peter  
dc.date.available
2023-12-05T15:04:25Z  
dc.date.issued
2018-11  
dc.identifier.citation
Poulhazan, Pierre Antoine; Scannapieco, Cecilia; Creasey, Peter; Precision pollution - The effects of enrichment yields and timing on galactic chemical evolution; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 480; 4; 11-2018; 4817-4841  
dc.identifier.issn
0035-8711  
dc.identifier.uri
http://hdl.handle.net/11336/219346  
dc.description.abstract
We present an update to the chemical enrichment component of the smoothed-particle hydrodynamics model for galaxy formation presented in Scannapieco et al. (2005) in order to address the needs of modelling galactic chemical evolution in realistic cosmological environments. Attribution of the galaxy-scale abundance patterns to individual enrichment mechanisms such as the winds from asymptotic giant branch (AGB) stars or the presence of a prompt fraction of type Ia supernovae (SNe) is complicated by the interaction between them and gas cooling, subsequent star formation, and gas ejection. In this work, we address the resulting degeneracies by extending our implementation to a suite of mechanisms that encompasses different initial mass functions, models for yields from the aforementioned stars, models for the prompt component of the delay time distribution (DTD) for type Ia SNe and metallicity-dependent gas cooling rates, and then applying these to both isolated initial conditions and cosmological hydrodynamical zoom simulations. We find DTDs with a large prompt fraction (such as the bimodal and power-law models) have, at $z$ = 0, similar abundance patterns compared to the low-prompt component time distributions (uniform or wide Gaussian models). However, some differences appear, such as the former having systematically higher [X/Fe] ratios and narrower [O/Fe] distributions compared to the latter, and a distinct evolution of the [Fe/H] abundance.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
Wiley Blackwell Publishing, Inc  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
COSMOLOGY: THEORY  
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GALAXIES: EVOLUTION  
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GALAXIES: FORMATION  
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GALAXIES: STRUCTURE  
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METHODS: NUMERICAL  
dc.subject.classification
Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
Precision pollution - The effects of enrichment yields and timing on galactic chemical evolution  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2023-12-04T10:13:58Z  
dc.journal.volume
480  
dc.journal.number
4  
dc.journal.pagination
4817-4841  
dc.journal.pais
Reino Unido  
dc.journal.ciudad
Londres  
dc.description.fil
Fil: Poulhazan, Pierre Antoine. Leibniz Institut Fuer Astrophysik Potsdam; Alemania  
dc.description.fil
Fil: Scannapieco, Cecilia. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria; Argentina  
dc.description.fil
Fil: Creasey, Peter. University of California; Estados Unidos  
dc.journal.title
Monthly Notices of the Royal Astronomical Society  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/480/4/4817/5066176  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/https://doi.org/10.1093/mnras/sty2080  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1808.00007