Evolution of the Mass-Metallicity Relation from IMAGES

Details Evolution of the Mass-Metallicity Relation from IMAGES Evolution of the Mass-Metallicity Relation from IMAGES

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..390..318r&link_type=abstract

Pathways Through an Eclectic Universe ASP Conference Series, Vol. 390, proceedings of the conference held 23-27 April, 2007 at S

Statistics

Methodology

2

Scientific paper

The evolution of the stellar mass-metallicity relation is still a matter of intense debate tep*{Savaglio05,Liang06}. We present here preliminary results using a sample of intermediate mass galaxies with redshift between 0.4 and 0.8. We take special care of the methodology used to measure metallicity in order to avoid any systematic errors coming from bad flux measurement or unreliable extinction determination. We confirm the results of Liang et al. (2006) that at z˜ 0.6, galaxies have gas phases a half less enriched than in the local Universe.

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