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astro-ph.SR2025
Is a 1D perturbative method sufficient for asteroseismic modelling of Cephei pulsators? Implications for measurements of rotation and internal magnetic fields
J. S. G. Mombarg, V. Vanlaer, S. B. Das +6
Asymmetries in the observed rotational splittings of a multiplet contain information about the star's rotation profile and internal magnetic field. However, to exploit this informa…
astro-ph.SR2025
An Educational Guide for 2D Stellar Structure Calculations of Rapidly Rotating Stars using the ESTER code
Russel White, Jane Pratt, Michel Rieutord
The Evolution STEllaire en Rotation (ESTER) code is the first 2D stellar structure code to be made open-source and freely available to the astronomy and astrophysics community. An…