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The elemental abundance of quiescent galaxies in the LEGA-C survey: the (non-)evolution of [α/Fe] from z = 0.75 to z = 0

We measure the [α/Fe] abundances for 183 quiescent galaxies at z = 0.60−0.75 with stellar masses ranging 10.4 ≤ log10(M*/M⊙) ≤ 11.6 selected from the Large Early Galaxy Astrophysics Census survey. We estimate [α/Fe] from the ratio of the spectral indices Mgb (λ ∼ 5177 Å) and Fe4383, compared to pre...

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Main Authors: Bevacqua, Davide (Author) , Saracco, Paolo (Author) , La Barbera, Francesco (Author) , D’Ago, Giuseppe (Author) , De Propris, Roberto (Author) , Ferreras, Ignacio (Author) , Gallazzi, Anna (Author) , Pasquali, Anna (Author) , Spiniello, Chiara (Author)
Format: Article (Journal)
Language:English
Published: November 2023
In: Monthly notices of the Royal Astronomical Society
Year: 2023, Volume: 525, Issue: 3, Pages: 4219-4230
ISSN:1365-2966
DOI:10.1093/mnras/stad2403
Online Access:Verlag, kostenfrei, Volltext: https://doi.org/10.1093/mnras/stad2403
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Author Notes:Davide Bevacqua, Paolo Saracco, Francesco La Barbera, Giuseppe D’Ago, Roberto De Propris, Ignacio Ferreras, Anna Gallazzi, Anna Pasqual and Chiara Spiniello
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Summary:We measure the [α/Fe] abundances for 183 quiescent galaxies at z = 0.60−0.75 with stellar masses ranging 10.4 ≤ log10(M*/M⊙) ≤ 11.6 selected from the Large Early Galaxy Astrophysics Census survey. We estimate [α/Fe] from the ratio of the spectral indices Mgb (λ ∼ 5177 Å) and Fe4383, compared to predictions of simple stellar population models. We find that 91 per cent of quiescents in our sample have supersolar [α/Fe], with an average value of [α/Fe] = +0.24 ± 0.01. We find no significant correlation between [α/Fe] and stellar metallicity, mass, velocity dispersion, and average formation time. Galaxies that formed the bulk of their stellar mass on time-scales shorter than 1 Gyr follow the same [α/Fe] distribution as those which formed on longer time-scales. In comparison to local early-type galaxies and to stacked spectra of quiescent galaxies at z = 0.38 and z = 0.07, we find that the average [α/Fe] has not changed between z = 0.75 and the present time. Our work shows that the vast majority of massive quiescent galaxies at z ∼ 0.7 are α-enhanced, and that no detectable evolution of the average [α/Fe] has taken place over the last ∼6.5 Gyr.
Item Description:Veröffentlicht: 31. August 2023
Gesehen am 25.06.2024
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stad2403

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