Issue |
A&A
Volume 447, Number 1, February III 2006
|
|
---|---|---|
Page(s) | 113 - 119 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20053821 | |
Published online | 27 January 2006 |
Significant evolution of the stellar mass-metallicity relation since z ~ 0.65
1
National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, PR China e-mail: ycliang@bao.ac.cn
2
GEPI, Observatoire de Paris-Meudon, 92195 Meudon, France
Received:
13
July
2005
Accepted:
21
September
2005
We present the stellar mass-metallicity relation for 34 galaxies selected from CFRS and Marano fields, and compare it to those
derived from three local samples of galaxies (NFGS, KISS and SDSS). Our metal
abundance estimates account for extinction effects, as estimated from
IR/optical ratios and Balmer line ratios. All three comparisons show that the
intermediate mass galaxies at
are more metal-deficient by
0.3 dex at a given MK or stellar mass relative to
. We find no evidence
that this discrepancy could be related to different methods used to derive mass
and metallicity. Assuming a closed box model predicts a gas fraction converted
into stars of 20–25% since
, if the gas fraction is 10–20% in
present-day galaxies with intermediate masses. This result is in excellent
agreement with previous findings that most of the decline of the cosmic star
formation density is related to the population of intermediate mass galaxies,
which is composed of 75% spirals today. We find no evidence for a change of
the slope of the Mstar–Z relation from
to
within the
intermediate mass range (
).
Key words: galaxies: abundances / galaxies: evolution / galaxies: ISM / galaxies: spiral / galaxies: starburst / galaxies: stellar content
© ESO, 2006
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