---
res:
  bibo_abstract:
  - Observations show that star-forming galaxies reside on a tight 3D 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⊙ from the EAGLE hydrodynamical simulation to examine 3D 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 towards 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
  - foaf_Person:
      foaf_givenName: Joop
      foaf_name: Schaye, Joop
      foaf_surname: Schaye
  bibo_doi: 10.1093/mnrasl/sly093
  bibo_issue: '1'
  bibo_volume: 479
  dct_date: 2018^xs_gYear
  dct_isPartOf:
  - http://id.crossref.org/issn/1745-3925
  - http://id.crossref.org/issn/1745-3933
  dct_language: eng
  dct_publisher: Oxford University Press@
  dct_subject:
  - Space and Planetary Science
  - Astronomy and Astrophysics
  - 'galaxies: abundances'
  - 'galaxies: evolution'
  - 'galaxies: formation'
  - 'galaxies: star formation'
  dct_title: Star-forming galaxies are predicted to lie on a fundamental plane of
    mass, star formation rate, and α-enhancement@
...