The NIRVANDELS Survey: a robust detection of α-enhancement in star-forming galaxies at z 3.4
dc.contributor.author | Cullen, F. | |
dc.contributor.author | Shapley, A. | |
dc.contributor.author | McLure, R. | |
dc.contributor.author | Dunlop, J.S | |
dc.contributor.author | Sanders, R.L | |
dc.contributor.author | Topping, M.W | |
dc.contributor.author | Reddy, N.A | |
dc.contributor.author | Amorin, R. | |
dc.contributor.author | Begley, R. | |
dc.contributor.author | Bolzonella, M. | |
dc.contributor.author | Calabro, A. | |
dc.contributor.author | Carnall, A.C | |
dc.contributor.author | Castellano, M. | |
dc.contributor.author | Cimatti, A. | |
dc.contributor.author | Cirasuolo, M. | |
dc.contributor.author | Cresci, G. | |
dc.contributor.author | Fontana, A. | |
dc.contributor.author | Fontanot, F. | |
dc.contributor.author | Garilli, B. | |
dc.contributor.author | Guaita, L. | |
dc.contributor.author | Hamadouche, M. | |
dc.contributor.author | Hathi, N.P | |
dc.contributor.author | Mannucci, F. | |
dc.contributor.author | McLeod, D. J | |
dc.contributor.author | Pentericci, L. | |
dc.contributor.author | Saxena, A. | |
dc.contributor.author | Talia, M. | |
dc.contributor.author | Zamorani, G. | |
dc.date.accessioned | 2021-07-09T16:41:46Z | |
dc.date.available | 2021-07-09T16:41:46Z | |
dc.date.issued | 2021-05 | |
dc.description | Indexación: Scopus | es |
dc.description.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∗. © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. | es |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society Open Access Volume 505, Issue 1, Pages 903 - 9201 July 2021 | es |
dc.identifier.issn | 00358711 | |
dc.identifier.uri | http://repositorio.unab.cl/xmlui/handle/ria/19336 | |
dc.language.iso | en | es |
dc.publisher | Oxford University Press | es |
dc.title | The NIRVANDELS Survey: a robust detection of α-enhancement in star-forming galaxies at z 3.4 | es |
dc.type | Artículo | es |
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