collaborators

5 papers

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.SR2026

Multiplicity of Massive stars in the Milky Way (M3W). I. Project description, UNWIND, application to GLS 11 448, and DIB catalog

J. Maíz Apellániz, R. C. Gamen, G. Holgado +8

(ABRIDGED BUT NOT TOO FAR) Multiplicity is ubiquitous among massive stars and its understanding is constrained by the sample of well-determined orbits. The immediate goal of M3W is…

astro-ph.SR2026

Magnetic field detections in massive systems at different stages of interaction

S. Hubrig, M. Abdul-Masih, S. P. Jarvinen +4

Despite the importance of magnetic fields in massive stars, their origin is widely debated and still not well understood. With the mounting evidence for the importance of studying…

astro-ph.SR2024

Observations of massive contact binaries in the local universe

Michael Abdul-Masih

The contact phase represents a crossroad in the evolution of massive binary stars. Depending on the internal physics, the predicted end products can vary greatly including various…

astro-ph.SR2024

Magnetic massive stars: confirming the merger scenario for the magnetic field generation

Swetlana Hubrig, Markus Schöller, Silva P. Järvinen +4

Magnetic fields are considered to be key components of massive stars, with a far-reaching impact on their evolution and ultimate fate. A magnetic mechanism was suggested for the co…