activity
20042025
most citedSpin down of the core rotation in red giants

463 citations · 1.9k across the 25 of their papers we have counts for

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20 papers · 1 filter

astro-ph.SR2025

Cesam2k20: A code for a new generation of stellar evolution models. I. Description of the code

L. Manchon, M. Deal, J. P. C. Marques +1

We present Cesam2k20, the latest version of the hydrostatic stellar evolution code CESAM originally developed by P. Morel and collaborators. Over the last three decades, it has und…

astro-ph.SR2025★ 4 cited

The efficiency of mixed modes for angular momentum transport

Beatriz Bordadágua, Felix Ahlborn, Quentin Coppée +3

Core rotation rates of red-giant stars inferred from asteroseismic observations are substantially lower than predicted by current stellar models. This indicates the lack of an effi…

astro-ph.SR2020★ 9 cited

Analysis of eclipsing binaries in multiple stellar systems: the case of V1200 Centauri

F. Marcadon, K. G. Hełminiak, J. P. Marques +5

We present a new analysis of the multiple star V1200 Centauri based on the most recent observations for this system. We used the photometric observations from the Solaris network a…

astro-ph.SR2019★ 16 cited

Chemical mixing in low mass stars: I. Rotation against atomic diffusion including radiative accelerations

M. Deal, M-J. Goupil, J. P. Marques +2

When modelling stars with masses larger than 1.2Msun with no observed chemical peculiarity, atomic diffusion is often neglected because, on its own, it causes unrealistic surface a…

astro-ph.SR2018★ 18 cited

Influence of metallicity on the near-surface effect on oscillation frequencies

L. Manchon, K. Belkacem, R. Samadi +4

The CoRoT and Kepler missions have provided high-quality measurements of the frequency spectra of solar-like pulsators, enabling us to probe stellar interiors with a very high degr…

astro-ph.SR2018★ 77 cited

Impacts of radiative accelerations on solar-like oscillating main-sequence stars

M. Deal, G. Alecian, Y. Lebreton +5

Chemical element transport processes are among the crucial physical processes needed for precise stellar modelling. Atomic diffusion by gravitational settling nowadays is usually t…