---
res:
  bibo_abstract:
  - "Observations show that star-forming galaxies reside on a tight three-dimensional
    plane between mass, gas-phase metallicity and star formation rate (SFR), which
    can be explained by the interplay between metal-poor gas inflows, SFR and outflows.
    However, different metals are released on different time-scales, which may affect
    the slope of this relation. Here, we use central, star-forming galaxies with Mstar
    = 109.0−10.5 M\f from the EAGLE hydrodynamical simulation to examine three-dimensional
    relations between mass, SFR and chemical enrichment using absolute and relative
    C, N, O and Fe abundances. We show that the scatter is smaller when gas-phase
    α-enhancement is used rather than metallicity. A similar plane also exists for
    stellar α-enhancement, implying that present-day specific SFRs are correlated
    with long time-scale star formation histories. Between z = 0 and 1, the α-enhancement
    plane is even more insensitive to redshift than the plane using metallicity. However,
    it evolves at z > 1 due to lagging iron yields. At fixed mass, galaxies with higher
    SFRs have star formation histories shifted toward late times, are more α-enhanced
    and this α-enhancement increases with redshift as observed. These findings suggest
    that relations between physical properties inferred from observations may be affected
    by systematic variations in α-enhancements.@eng"
  bibo_authorlist:
  - foaf_Person:
      foaf_givenName: Jorryt J
      foaf_name: Matthee, Jorryt J
      foaf_surname: Matthee
      foaf_workInfoHomepage: http://www.librecat.org/personId=7439a258-f3c0-11ec-9501-9df22fe06720
    orcid: 0000-0003-2871-127X
  bibo_doi: 10.1038/s41550-021-01415-y
  bibo_volume: 5
  dct_date: 2021^xs_gYear
  dct_isPartOf:
  - http://id.crossref.org/issn/2397-3366
  dct_language: eng
  dct_publisher: Springer Nature@
  dct_subject:
  - Astronomy and Astrophysics
  - galaxies
  - formation - galaxies
  - evolution - galaxies
  - star formation - galaxies
  - abundances
  dct_title: Differences in galaxy colours are not just about the mass@
...