Journal Article

The cosmic evolution of metallicity from the SDSS fossil record

Benjamin Panter, Raul Jimenez, Alan F. Heavens and Stephane Charlot

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 391, issue 3, pages 1117-1126
Published in print December 2008 | ISSN: 0035-8711
Published online November 2008 | e-ISSN: 1365-2966 | DOI: https://dx.doi.org/10.1111/j.1365-2966.2008.13981.x
The cosmic evolution of metallicity from the SDSS fossil record

Show Summary Details

Preview

We infer the time evolution of the stellar metallicity for Sloan Digital Sky Survey (SDSS) galaxies by interpreting their spectra through stellar population models using a sample that spans 5 orders of magnitude in stellar mass (). Assuming the Bruzual & Charlot stellar population models, we find that more massive galaxies are more metal rich than less massive ones at all redshifts; the mass–metallicity relation is imprinted in galaxies from z∼ 3, close to the epoch of formation. For galaxies with present stellar masses >1010M, the time evolution of stellar metallicity is very weak, with at most dex shift over 12 Gyr – for this reason, the mass–metallicity relation evolves little with redshift. However, for galaxies with present stellar masses <1010M, the evolution is significant, with metallicity increasing by more than a decade from redshift 3 to the present. By being able to recover the metallicity history, we have managed to identify the origin of a recent discrepancy between the metallicity recovered from nebular lines and absorption lines. As expected, we show that the young population dominates the former while the old population the latter. We have investigated the dependence on the stellar models used and find that older stellar population synthesis codes do not produce a clear result. Finally, we have explored the relationship between cluster environment and metallicity, and find a strong correlation in the sense that galaxies in high-density regions have high metallicity.

Keywords: galaxies: abundances; galaxies: evolution; galaxies: statistics

Journal Article.  6691 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.