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19992026
most citedGamma-ray emission from Wolf-Rayet binaries

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

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19 papers · 1 filter

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.HE2024

Study of Wolf-Rayet stars using uGMRT

Anindya Saha, Anandmayee Tej, Santiago del Palacio +4

In recent years, systems involving massive stars with large wind kinetic power have been considered as promising sites for investigating relativistic particle acceleration in low r…

astro-ph.HE2024★ 3 cited

Investigating the Role of Pre-supernova Massive Stars in the Acceleration of Galactic Cosmic Rays

Michael De Becker, Santiago del Palacio, Paula Benaglia +5

Galactic cosmic rays (GCRs) constitute a significant part of the energy budget of our Galaxy, and the study of their accelerators is of high importance in modern astrophysics. Thei…

astro-ph.HE2023

Search for particle acceleration in two massive Wolf-Rayet stars using uGMRT observations

Anindya Saha, Anandmayee Tej, Santiago del Palacio +4

Large wind kinetic power of Wolf-Rayet (WR) stars make them ideal targets in low radio frequencies to search for non-thermal emission due to relativistic particle acceleration. In…