collaborators

7 papers

astro-ph.SR2026

On the feasibility of inverting the rotation of the solar core with mixed f/g modes

Armand Leclerc, Arthur Le Saux, J. M. Joel Ong +1

Context: Thanks to helioseismology, the rotation profile of the Sun has been measured with great precision down to 20% of its total radius. This rotation profile is used as a calib…

astro-ph.SR2026

Asteroseismic imprints of strong non-axisymmetric fields in the cores of red giants

Nicholas Z. Rui, J. M. Joel Ong, Armand Leclerc +5

To date, magnetic fields have been asteroseismically measured in nearly one hundred red giant cores. However, most analyses assume weak magnetic fields and slow rotation so that pe…

astro-ph.SR2026

Extending asteroseismic magnetometry across the diverse landscape of magnetic structures

Nicholas Z. Rui, J. M. Joel Ong, Armand Leclerc +6

Magnetic fields have now been asteroseismically measured in the cores of many red giants. However, most interpretations of these measurements assume that the magnetic field is far…

astro-ph.SR2026

Revealing mixed modes in compressible hydrodynamical simulations of red giant stars

Nils B. de Vries, Arthur Le Saux, Isabelle Baraffe +4

Mixed modes are observed in many low-mass evolved stars. They provide information about core rotation rates of these stars, which are lower than predicted by stellar evolution mode…

astro-ph.EP2025

Radial modes of pressure bumps and dips in astrophysical discs

Armand Leclerc, Guillaume Laibe, Elliot Lynch +1

This study investigates the signatures of pressure extrema on global oscillations in discs. To this end, we use the framework of wave topology to establish a generalised local disp…

astro-ph.SR2025

A core-sensitive mixed / mode of the Sun predicted by wave topology and hydrodynamical simulation

Arthur Le Saux, Armand Leclerc, Guillaume Laibe +2

Helioseismology has revolutionized our understanding of the Sun by analyzing its global oscillation modes. However, the solar core remains elusive, limiting a full understanding of…