Chemical evolution of galaxies in the high redshift universe

María Emilia De Rossi, Patricia Beatriz Tissera

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

In this work, we present preliminary results on the chemical evolution of galaxies at 3 < z < 7 in cosmological simulations. The simulated mass-metallicity relation (MZR) predicted by the adopted supernova (SN) feedback model is consistent with recent observations. However, our findings suggest that the parameters which regulate the SN feedback efficiency need to be revised in order to reproduce the observed evolution of the MZR towards z ∼ 0.

Original languageEnglish
Title of host publicationFirst Stars and Galaxies
Subtitle of host publicationChallenges for the Next Decade
Pages279-280
Number of pages2
DOIs
Publication statusPublished - 2010
Event1st Stars and Galaxies: Challenges for the Next Decade - Austin, TX, United States
Duration: 8 Mar 201011 Mar 2010

Publication series

NameAIP Conference Proceedings
Volume1294
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

Other1st Stars and Galaxies: Challenges for the Next Decade
Country/TerritoryUnited States
CityAustin, TX
Period8/03/1011/03/10

Keywords

  • Chemical abundances
  • Cosmology
  • Galaxy formation
  • High redshift

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Fingerprint

Dive into the research topics of 'Chemical evolution of galaxies in the high redshift universe'. Together they form a unique fingerprint.

Cite this