collaborators

6 papers

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…

astro-ph.GA2025

High resolution radio analysis of the starburst galaxy NGC 4527: signatures of an AGN core

C. A. Galante, G. E. Romero, J. Saponara +1

NGC 4527 is a nearby edge-on spiral galaxy with both starburst and AGN features, hosting a LINER nucleus. We present a radio study of the large-scale structure and nuclear region o…

astro-ph.SR2025

Radio study of the colliding wind binary HD93129A near periastron and its surroundings

Paula Benaglia, Santiago del Palacio, Juliana Saponara +3

HD93129A is an O+O stellar system whose CWR has been mapped by high angular resolution observations at cm wavelengths. The synchrotron nature of the radio emission confirms its par…