Evolution of the luminosity-metallicity-stellar mass correlation in a hierarchical scenario

M. E. De Rossi, P. B. Tissera, C. Scannapieco

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

Abstract

We study the evolution of the Stellar Mass-Metallicity Relation and the Luminosity-Metallicity Relation by performing numerical simulations in a cosmological framework. We find that the slope and the zero point of the Luminosity-Metallicity Relation evolve in such a way that, at a given metallicity, systems were ∼3 mag brighter at z = 3 compared to galaxies in the local universe, which is consistent with the observational trend. The local Stellar Mass-Metallicity Relation shows also a good agreement with recent observations. We identify a characteristic stellar mass Mc ∼ 1010.2 M⊙h-1 at which the slope of the Stellar Mass-Metallicity Relation decreases for larger stellar masses. Our results indicate that Mc arises naturally as a consequence of the hierarchical building up of the structure.

Original languageEnglish
Title of host publicationGroups of Galaxies in the Nearby Universe
Subtitle of host publicationProceedings of the ESO Workshop held at Santiago de Chile, December 5-9, 2005
EditorsIvo Saviane, Valentin Ivanov, Jordanka Borissova
Pages243-245
Number of pages3
DOIs
Publication statusPublished - 2007

Publication series

NameESO Astrophysics Symposia
Volume2007
ISSN (Print)1431-2433
ISSN (Electronic)1611-6143

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Physics and Astronomy (miscellaneous)

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