135 citations · 826 across the 25 of their papers we have counts for
26 papers
The Potential Contribution of Radiative Supernova Remnants to the Local Cosmic Ray Spectrum
P. Cristofari, V. H. M. Phan, S. Recchia +1
Recent observations of very-high-energy gamma rays from massive stellar clusters and microquasars have demonstrated that these systems can efficiently accelerate particles to very…
Wolf-Rayet stars as tracers of gamma-ray emission: Isolated stars and stellar clusters/associations
Alexandre Inventar, Giada Peron, Sarah Recchia +1
Context: Recent gamma-ray observations of young star clusters revealed that stellar wind termination shocks accelerate particles, with the energy reservoir provided by the mechanic…
Dust-driven streaming instability and magnetic field amplification downstream of supernova remnant shocks
S. Gabici, J. C. Raymond, A. Ciardi +3
The acceleration of cosmic rays up to PeV energies at supernova remnant shocks requires an amplification of the ambient magnetic field. The amplification mechanism must operate ups…
Gamma-rays from Wolf-Rayet stellar winds
A. Inventar, G. Peron, S. Recchia +1
Gamma-ray observations of young star clusters have recently provided evidence for particle acceleration occurring at stellar wind termination shocks, fueled by the mechanical energ…
Can cosmic rays explain the high ionisation rates in the Galactic centre?
Sruthiranjani Ravikularaman, Sarah Recchia, Vo Hong Minh Phan +1
The Central Molecular Zone (CMZ), located in the centre of the Milky Way, is a roughly cylindrical structure of molecular gas extending up to parsecs around the supermassive black…
Cosmic rays cannot explain the high ionisation rates in the Galactic centre
Sruthiranjani Ravikularaman, Sarah Recchia, Vo Hong Minh Phan +1
The H ionisation rate in the central molecular zone, located in the Galactic centre, is estimated to be , based on observations of H…