S Vercellone, C Bigongiari, A Burtovoi… - Journal of High Energy …, 2022 - Elsevier
Abstract The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project led by the Italian National Institute for Astrophysics (INAF) is developing and will deploy at the …
Observations of the Milky Way at TeV–PeV energies reveal a bright diffuse flux of hadronic cosmic rays and also bright point sources of gamma rays. If the gamma-ray sources are …
Energetic non-thermal particles, or cosmic rays, are a major component of astrophysical plasmas next to magnetic fields, radiation, and thermal gas. Cosmic rays are usually sub …
We present the serendipitous detection of a new Galactic supernova remnant (SNR), G288. 8–6.3, using data from the Australian Square Kilometre Array Pathfinder (ASKAP) …
Context. The properties of the population of Galactic supernova remnants (SNRs) are essential to our understanding of the dynamics of the interstellar medium (ISM) in the Milky …
R Brose, I Sushch, J Mackey - Monthly Notices of the Royal …, 2022 - academic.oup.com
Supernova remnants (SNRs) are known to accelerate cosmic rays from the detection of non- thermal emission in radio waves, X-rays, and gamma-rays. However, the ability to accelerate …
R Brose, M Pohl, I Sushch - Astronomy & Astrophysics, 2021 - aanda.org
Context. Supernova remnants (SNRs) are known to accelerate particles to relativistic energies, on account of their nonthermal emission. The observational progress from radio to …
Context. Galactic cosmic rays (CRs) are widely assumed to arise from diffusive shock acceleration, specifically at shocks in supernova remnants (SNRs). These shocks expand in …
F Acero, A Acharyya, R Adam, A Aguasca-Cabot… - Astroparticle …, 2023 - Elsevier
Abstract The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such …