activity
20222026
most citedTime evolution of Ce as traced by APOGEE using giant stars observed with the Kepler, TESS and K2 missions

13 citations · 47 across the 13 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2026

Extra modes in helium-core-burning stars probing an infra core cavity

B. Mosser, M. Takata, C. Pinçon +5

Dipole mixed modes observed in the oscillation pattern of red giant stars probe the radiative regions in the stellar core. Oscillation spectra of helium-core-burning stars sometime…

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★ 2 cited

Predictions of gravity mode pulsations of collisional blue straggler stars in globular clusters

Lorenzo Briganti, Walter Eduard van Rossem, Andrea Miglio +2

Blue straggler stars (BSSs) are exotic objects, which, being the results of processes such as mass transfer, mergers, or collisions, are considered key objects in the study of thei…

astro-ph.SR2025★ 2 cited

Inferring the efficiency of convective-envelope overshooting in Red Giant Branch stars

Lorenzo Briganti, Marco Tailo, Edoardo Ceccarelli +6

The understanding of mixing processes in stars is crucial for improving our knowledge of the chemical abundances in stellar photospheres and of their variation with evolutionary ph…

astro-ph.SR2025★ 4 cited

Parametric models of core-helium-burning stars: structural glitches near the core

Massimiliano Matteuzzi, Gaël Buldgen, Marc-Antoine Dupret +3

Understanding the internal structure of core helium burning (CHeB) stars is crucial for evaluating transport processes in nuclear-burning regions, constructing accurate stellar pop…

astro-ph.SR2025★ 7 cited

DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations

A. Mazzi, J. S. Thomsen, A. Miglio +5

Asteroseismology gives us the opportunity to better characterize binaries and their products, and shed light on their role in Galactic populations. We estimate occurrence rates, ma…

astro-ph.SR2025★ 7 cited

Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary

J. S. Thomsen, A. Miglio, K. Brogaard +26

The study of resonant oscillation modes in low-mass red giant branch stars enables their ages to be inferred with exceptional (10%) precision, unlocking the possibility to re…

astro-ph.SR2024★ 7 cited

Anomalously low-mass core-He-burning star in NGC 6819 as a post-common-envelope phase product

Massimiliano Matteuzzi, David Hendriks, Robert G. Izzard +5

Precise masses of red-giant stars enable a robust inference of their ages, but there are cases where these age estimates are highly precise yet very inaccurate. Examples are core-h…

astro-ph.SR2024★ 5 cited

The true nature of HE0057-5959, the most metal-poor Li-rich star

A. Mucciarelli, P. Bonifacio, L. Monaco +2

The Li-rich stars are a class of rare objects with A(Li) higher than that of other stars in the same evolutionary stage. Their origin is still debated and valuable routes are the C…