activity
20072026
most citedStrong evidences of hadron acceleration in Tycho's Supernova Remnant

277 citations · 3.5k across the 94 of their papers we have counts for

collaborators

100 papers

astro-ph.HE2026

Investigating signatures of extinct PeVatron activity in supernova remnants IC 443 and W51 C

Silvia Celli, Giovanni Morlino

Context. Supernova remnants (SNRs) are renewed sources of non-thermal particles and the main contributors of Galactic cosmic rays (CRs). Recent ultra-high energy (UHE) gamma-ray da…

astro-ph.HE2026

Supernova remnants in the new radio astronomy era

A. Ingallinera, M. Arias, G. Castelletti +25

Supernova remnants (SNRs) are what is left after stellar explosions, when the stellar ejecta, the explosion shock and the circumstellar medium interact. Despite being among the fir…

astro-ph.HE2026

A broadband view of the thermal and non-thermal emission from the embedded massive star cluster RCW 38

Giada Peron, Andrea Bracco, Giovanni Morlino +4

Gamma-ray emission has now been detected from a variety of source classes in the Galaxy, including clusters of young massive stars. RCW 38, a very young embedded massive star clust…

astro-ph.HE2026

Particle acceleration at recollimation shocks in sub-relativistic jets. A model for jets in Seyfert Galaxies, Microquasars and Protostellar Systems

Enrico Peretti, Elena Amato, Silvio Sergio Cerri +3

Growing observational evidence suggests that subrelativistic (SR) astrophysical jets may accelerate particles at slowly evolving standing shocks. Recollimation shocks (RCS) are exp…

astro-ph.HE2025★ 3 cited

Hadronic acceleration in the young star cluster NGC 6611 inside the M16 region unveiled by Fermi-LAT: constraints on the acceleration efficiency

Giada Peron, Stefano Menchiari, Giovanni Morlino +1

Context. Young Massive Star Clusters, long considered as potentially important sources of galactic cosmic rays, have recently emerged as gamma-ray emitters up to very high energies…

astro-ph.HE2025★ 1 cited

Massive star clusters in the gamma-ray sky: the role of HII regions

Giada Peron, Giovanni Morlino, Stefano Gabici +1

Massive Star Clusters (SCs) have been proposed as important CR sources, with the potential of explaining the high-energy end of the Galactic cosmic-ray (CR) spectrum, that Supernov…