---
res:
  bibo_abstract:
  - "Context. γ Dor stars are ideal targets for studies of the innermost dynamical
    properties of stars, due to their rich asteroseismic spectrum of gravity modes.
    Integrating internal magnetism to the picture appears as the next milestone of
    detailed asteroseismic studies, for its prime importance on stellar evolution.
    The inertial dip in prograde dipole modes period-spacing pattern of γ Dors stands
    out as a unique window on the convective core structure and dynamics. Recent studies
    have highlighted the dependence of the dip structure on core density stratification,
    the contrast of the near-core Brunt-Väisälä frequency and rotation rate, as well
    as the core-to-near-core differential rotation. In addition, the effect of envelope
    magnetism has been derived on low-frequency magneto-gravito-inertial waves.\r\n\r\nAims.
    We revisited the inertial dip formation including core and envelope magnetism,
    and explored the probing power of this feature on dynamo-generated core fields.\r\n\r\nMethods.
    We considered as a first step a toroidal magnetic field with a bi-layer (core
    and envelope) Alfvén frequency. This configuration allowed us to revisit the coupling
    problem using our knowledge on both core magneto-inertial modes and envelope magneto-gravito-inertial
    modes. Using this configuration, we were able to stay in an analytical framework
    to exhibit the magnetic effects on the inertial dip shape and location. This configuration
    allowed a laboratory to be set up that moves us towards the comprehension of magnetic
    effects on the dip structure.\r\n\r\nResults. We show a shift of the inertial
    dip towards lower spin parameter values and a thinner dip with increasing core
    magnetic field’s strength, quite similar to the signature of differential rotation.
    The magnetic effects become sizeable when the ratio of the magnetic to the Coriolis
    effects is high enough. We explored the potential degeneracy of the magnetic effects
    with differential rotation. We studied the detectability of core magnetism, considering
    both observational constraints on the periods of the modes and potential gravito-inertial
    mode suppression.@eng"
  bibo_authorlist:
  - foaf_Person:
      foaf_givenName: Lucas
      foaf_name: Barrault, Lucas
      foaf_surname: Barrault
      foaf_workInfoHomepage: http://www.librecat.org/personId=4471a8fd-32c1-11ee-a9a4-fb670d398f64
  - foaf_Person:
      foaf_givenName: Lisa Annabelle
      foaf_name: Bugnet, Lisa Annabelle
      foaf_surname: Bugnet
      foaf_workInfoHomepage: http://www.librecat.org/personId=d9edb345-f866-11ec-9b37-d119b5234501
    orcid: 0000-0003-0142-4000
  - foaf_Person:
      foaf_givenName: S.
      foaf_name: Mathis, S.
      foaf_surname: Mathis
  - foaf_Person:
      foaf_givenName: J. S.G.
      foaf_name: Mombarg, J. S.G.
      foaf_surname: Mombarg
  bibo_doi: 10.1051/0004-6361/202555213
  bibo_volume: 701
  dct_date: 2025^xs_gYear
  dct_identifier:
  - UT:001585834500002
  dct_isPartOf:
  - http://id.crossref.org/issn/0004-6361
  - http://id.crossref.org/issn/1432-0746
  dct_language: eng
  dct_publisher: EDP Sciences@
  dct_title: 'Exploring the probing power of γ Dor''s inertial dip for core magnetism:
    The case of a toroidal field@'
...