collaborators

8 papers

astro-ph.SR2026

Investigating the impact of Solar Fusion III reaction rates on helioseismic constraints and solar neutrino fluxes

T. Sandron, G. Buldgen, A. Noels +2

Nuclear reaction rates are crucial ingredients of solar and stellar models, they directly impact the duration of the life of stars and the energy they produce. In the solar case, t…

astro-ph.SR2026

A data-driven estimate of the protosolar helium mass fraction

G. Buldgen, M. Kunitomo, A. Noels +3

The protosolar helium mass-fraction is a key ingredient of solar, planetary models and enrichment laws. However, the assumed values often rely on simplified descriptions of the tra…

astro-ph.SR2026

On the contradictory case of the binary system HD 81809 hosting two pulsating solar-like stars observed by TESS

Maria Pia Di Mauro, Camilla Pezzotti, Nuno Moedas +8

We present a new comprehensive study of HD81809, a nearby binary system of two solar-like stars showing high-amplitude X-ray emission and a well-defined 8-year solar-like magnetic…

astro-ph.SR2025

Detailed theoretical analysis of core Helium-burning stars: Mixed mode patterns I. Impact of the He-flash discontinuity and of induced semi-convection

L. Panier, G. Buldgen, M. Matteuzzi +4

Space missions like CoRoT, Kepler, and TESS have made asteroseismology a powerful probe of stellar interiors. Red giants are key targets thanks to their rich mixed-mode oscillation…

astro-ph.SR2025

The impact of the transport of chemicals and electronic screening on helioseismic and neutrino observations in solar models

Morgan Deal, Gaël Buldgen, Louis Manchon +3

The transport of chemical elements in stellar interiors is one of the greatest sources of uncertainties of solar and stellar modelling. The Sun, with its exquisite spectroscopic, h…

astro-ph.SR2025

Entropy proxy inversions as tracers of the evolution of physical conditions at the base of the solar convective envelope

G. Buldgen, A. Noels, V. A. Baturin +4

The Sun is an important calibrator for the theory of stellar structure and evolution. However, the accuracy of our solar evolution models is tightly linked to the physical ingredie…