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20232026
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astro-ph.SR2026

Detection of actinides in CEMP-rs stars

A. M. Riyas, D. Karinkuzhi, S. Van Eck +4

The carbon-enhanced metal-poor stars with hybrid enrichments of slow- and rapid neutron-capture elements, the so-called CEMP-rs stars, still raise many questions due to their elusi…

astro-ph.SR2026

Ages and ZAMS spin distribution of stars in detached eclipsing binaries

T. Merle, W. Van Rensbergen, L. Siess +4

Benchmarking fundamental stellar properties is essential for calibrating evolutionary models and establishing empirical relationships between mass, radius, luminosity and related s…

astro-ph.SR2026

The chemical fingerprint of the Gaia BH3 system. Evidence for early cluster enrichment from the analysis of 51 elements

Gregory Vanden Broeck, Thibault Merle, Nhat Tan Mai +5

The Gaia BH3 system hosts the most massive known stellar-origin black hole and a low-mass metal-poor companion whose chemical composition may constrain early explosive nucleosynthe…

astro-ph.SR2026

Stellar nucleosynthesis in the era of large surveys: S-process polluted binaries in GALAH DR4

A. Escorza, S. Vitali, D. Godoy-Rivera +11

Binary interactions during the AGB phase can lead to the formation of chemically peculiar stars with overabundances of s-process elements. Only a few hundreds of these stars have b…

astro-ph.SR2024

A new dimension in the variability of AGB stars: convection patterns size changes with pulsation

A. Rosales-Guzmán, J. Sanchez-Bermudez, C. Paladini +16

Stellar convection plays an important role in atmospheric dynamics, wind formation and the mass-loss processes in Asymptotic Giant Branch (AGB) stars. However, a direct characteriz…

astro-ph.SR2024

An impressionist view of V Hydrae. When MATISSE paints Asymmetric Giant Blobs

L. Planquart, C. Paladini, A. Jorissen +29

Our purpose is to study the effect of binary companions located within the first 10 stellar radii from the primary AGB star. In this work, we target the mass-losing carbon star V H…