Abstract
We present results from the NIRVANDELS survey on the gas-phase metallicity (Zg, tracing O/H) and stellar metallicity (Z∗, tracing Fe/H) of 33 star-forming galaxies at redshifts 2.95 < z < 3.80. Based on a combined analysis of deep optical and near-IR spectra, tracing the rest-frame far-ultraviolet (FUV; 1200-2000 Å) and rest-frame optical (3400-5500 Å), respectively, we present the first simultaneous determination of the stellar and gas-phase mass-metallicity relationships (MZRs) at z ≃ 3.4. In both cases, we find that metallicity increases with increasing stellar mass (M∗) and that the power-law slope at M∗ ≤ 1010M⊙ of both MZRs scales as Z ∝ M∗0.3. Comparing the stellar and gas-phase MZRs, we present direct evidence for super-solar O/Fe ratios (i.e. α-enhancement) at z > 3, finding (O/Fe) = 2.54 ± 0.38 × (O/Fe)⊙, with no clear dependence on M∗.
Original language | English |
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Pages (from-to) | 903-920 |
Number of pages | 18 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 505 |
Issue number | 1 |
DOIs | |
State | Published - Jul 1 2021 |
Bibliographical note
Publisher Copyright:© 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.
Funding
UK Science and Technology Facilities Council, 20173ML3WW 001 PRIN MIUR 2017, 1202007 ANID Fondecyt
Funders | Funder number |
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ANID Fondecyt | |
Science and Technology Facilities Council | 20173ML3WW 001 PRIN MIUR 2017 |
Keywords
- Galaxies: abundances
- Galaxies: high redshift
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science