---
res:
  bibo_abstract:
  - Magnetic fields can drastically change predictions of evolutionary models of massive
    stars via mass-loss quenching, magnetic braking, and efficient angular momentum
    transport, which we aim to quantify in this work. We use the MESA software instrument
    to compute an extensive main-sequence grid of stellar structure and evolution
    models, as well as isochrones, accounting for the effects attributed to a surface
    fossil magnetic field. The grid is densely populated in initial mass (3–60 M⊙),
    surface equatorial magnetic field strength (0–50 kG), and metallicity (representative
    of the Solar neighbourhood and the Magellanic Clouds). We use two magnetic braking
    and two chemical mixing schemes and compare the model predictions for slowly rotating,
    nitrogen-enriched (‘Group 2’) stars with observations in the Large Magellanic
    Cloud. We quantify a range of initial field strengths that allow for producing
    Group 2 stars and find that typical values (up to a few kG) lead to solutions.
    Between the subgrids, we find notable departures in surface abundances and evolutionary
    paths. In our magnetic models, chemical mixing is always less efficient compared
    to non-magnetic models due to the rapid spin-down. We identify that quasi-chemically
    homogeneous main sequence evolution by efficient mixing could be prevented by
    fossil magnetic fields. We recommend comparing this grid of evolutionary models
    with spectropolarimetric and spectroscopic observations with the goals of (i)
    revisiting the derived stellar parameters of known magnetic stars, and (ii) observationally
    constraining the uncertain magnetic braking and chemical mixing schemes.@eng
  bibo_authorlist:
  - foaf_Person:
      foaf_givenName: Z.
      foaf_name: Keszthelyi, Z.
      foaf_surname: Keszthelyi
  - foaf_Person:
      foaf_givenName: A. de
      foaf_name: Koter, A. de
      foaf_surname: Koter
  - foaf_Person:
      foaf_givenName: Ylva Louise Linsdotter
      foaf_name: Götberg, Ylva Louise Linsdotter
      foaf_surname: Götberg
      foaf_workInfoHomepage: http://www.librecat.org/personId=d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
    orcid: 0000-0002-6960-6911
  - foaf_Person:
      foaf_givenName: G.
      foaf_name: Meynet, G.
      foaf_surname: Meynet
  - foaf_Person:
      foaf_givenName: S. A.
      foaf_name: Brands, S. A.
      foaf_surname: Brands
  - foaf_Person:
      foaf_givenName: V.
      foaf_name: Petit, V.
      foaf_surname: Petit
  - foaf_Person:
      foaf_givenName: M.
      foaf_name: Carrington, M.
      foaf_surname: Carrington
  - foaf_Person:
      foaf_givenName: A. David-Uraz
      foaf_name: A. David-Uraz, A. David-Uraz
      foaf_surname: A. David-Uraz
  - foaf_Person:
      foaf_givenName: S. T.
      foaf_name: Geen, S. T.
      foaf_surname: Geen
  - foaf_Person:
      foaf_givenName: C.
      foaf_name: Georgy, C.
      foaf_surname: Georgy
  - foaf_Person:
      foaf_givenName: R.
      foaf_name: Hirschi, R.
      foaf_surname: Hirschi
  - foaf_Person:
      foaf_givenName: J.
      foaf_name: Puls, J.
      foaf_surname: Puls
  - foaf_Person:
      foaf_givenName: K. J.
      foaf_name: Ramalatswa, K. J.
      foaf_surname: Ramalatswa
  - foaf_Person:
      foaf_givenName: M. E.
      foaf_name: Shultz, M. E.
      foaf_surname: Shultz
  - foaf_Person:
      foaf_givenName: A. ud-Doula
      foaf_name: A. ud-Doula, A. ud-Doula
      foaf_surname: A. ud-Doula
  bibo_doi: 10.1093/mnras/stac2598
  bibo_issue: '2'
  bibo_volume: 517
  dct_date: 2022^xs_gYear
  dct_isPartOf:
  - http://id.crossref.org/issn/0035-8711
  - http://id.crossref.org/issn/1365-2966
  dct_language: eng
  dct_publisher: Oxford Academic@
  dct_title: 'The effects of surface fossil magnetic fields on massive star evolution:
    IV. Grids of models at solar, LMC, and SMC metallicities@'
...