activity
19992026
most citedGamma-ray emission from Wolf-Rayet binaries

114 citations · 1.3k across the 78 of their papers we have counts for

collaborators

78 papers

astro-ph.SR2026

Meerkat measurement of the radio emission from massive stars in the Galactic plane I. Wolf-Rayet stars

Mathilde Tasseroul, Michaël De Becker, Paula Benaglia +1

Massive stars, including Wolf-Rayet stars, are predominantly found in binary systems. These systems are known to emit both thermal emission from stellar winds and, occasionally, no…

astro-ph.HE2026

The influence of free-free absorption on the radio spectrum of Particle-Accelerating Colliding-Wind Binaries

Michaël De Becker, Agustina Belen Blanco, Mathilde Tasseroul +4

The study of massive stars in binary and higher-multiplicity systems that participate in particle acceleration is a key topic at the crossroads of massive star physics, shock physi…

astro-ph.HE2026

Enabling population studies on wind-driven Galactic binary systems

B. Marcote, P. Benaglia, V. Bosch-Ramon +8

Galactic binaries driven by stellar wind shocks, such as colliding wind binaries (CWBs) and gamma-ray binaries (gBs), harbor one of the most efficient particle acceleration engines…

astro-ph.HE2026

Investigating particle acceleration in the Wolf-Rayet bubble NGC 2359

Anindya Saha, Anandmayee Tej, Santiago del Palacio +4

Massive stars have been proposed as candidates to be major factories of Galactic cosmic rays (GCRs). However, this claim lacks enough empirical evidence, especially for isolated st…

astro-ph.SR2025

Thackeray's globules in IC 2944: the rocket effect revisited by ALMA

M. Fernández-López, L. A. Zapata, B. Reipurth +4

The prominent Thackeray's globules are a collection of cloudlets seen in silhouette against the bright emission of the IC 2944 HII region, ionized by the Collinder 249 cluster of e…

astro-ph.SR2025

Foreground and internal free-free absorption in particle-accelerating colliding-wind binaries : Insights from the radio emission of WR 147

M. Tasseroul, M. De Becker, A. B Blanco +2

Radio emission from massive binary systems is generally of composite nature, showing both a thermal emission component from the winds and a non-thermal component from relativistic…