23 citations · 23 across the 7 of their papers we have counts for
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The Missing MeV Window for Identifying Galactic PeVatrons: the need for a dedicated MeV Observatory
Martina Cardillo, Riccardo Campana, Yuri Evangelista +1
The identification of the sources responsible for accelerating Galactic cosmic-rays up to PeV energies remains a major open question in high-energy astrophysics. Recent observation…
Gamma-ray emission from particle illumination and shock-cloud interaction in the W51 Complex
Alan Sunny, Martina Cardillo
In the current era of very-high-energy (VHE) and ultra-high-energy (UHE) -ray astronomy, understanding Galactic PeVatrons and their acceleration mechanisms remains a primary obj…
The Origin of Multi-TeV Gamma-rays in LHAASO J0341+5258 via Cosmic Ray Illumination of Molecular Clouds
Abhijit Roy, Alan Sunny, Martina Cardillo +2
We investigate the origin of the ultra-high-energy -ray emission detected by the Large High Altitude Air Shower Observatory (LHAASO) from the source LHAASO J0341+5258, which has…
Studying SNR-MC interactions as galactic PeVatrons in the era of CTAO and ASTRI Mini-Array
Alan Sunny, Martina Cardillo, Antonio Tutone
Supernova remnants (SNRs) are widely recognized as key accelerators of Galactic cosmic rays (CRs), supported by the detection of the characteristic pion bump in the gamma-ray spect…
Supernova Remnants in Gamma Rays
Andrea Giuliani, Martina Cardillo
In the 1960s, the remnants of supernova explosions (SNRs) were indicated as a possible source of galactic cosmic rays through the Diffusive Shock Acceleration (DSA) mechanism. Sinc…
Gamma-rays and Neutrinos from Giant Molecular Cloud Populations in the Galactic Plane
Abhijit Roy, Jagdish C. Joshi, Martina Cardillo +3
The recent IceCube detection of significant neutrino flux from the inner Galactic plane has provided us valuable insights on the spectrum of cosmic rays in our Galaxy. This flux ca…
Investigating the high-frequency spectral features of SNRs Tycho, W44 and IC443 with the Sardinia Radio Telescope
S. Loru, A. Pellizzoni, E. Egron +20
The main characteristics in the radio continuum spectra of Supernova Remnants (SNRs) result from simple synchrotron emission. In addition, electron acceleration mechanisms can shap…