Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical …

M Ruszkowski, C Pfrommer - The Astronomy and Astrophysics Review, 2023 - Springer
Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …

[HTML][HTML] ASTRI Mini-Array core science at the Observatorio del Teide

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 …

Where are Milky Way's hadronic PeVatrons?

T Sudoh, JF Beacom - Physical Review D, 2023 - APS
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 …

[HTML][HTML] The cosmic ray-driven streaming instability in astrophysical and space plasmas

A Marcowith, AJ Van Marle, I Plotnikov - Physics of Plasmas, 2021 - pubs.aip.org
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 …

EMU Detection of a Large and Low Surface Brightness Galactic SNR G288. 8–6.3

MD Filipović, S Dai, B Arbutina… - The Astronomical …, 2023 - iopscience.iop.org
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) …

[HTML][HTML] A global view on star formation: The GLOSTAR Galactic plane survey-II. Supernova remnants in the first quadrant of the Milky Way

R Dokara, A Brunthaler, KM Menten, SA Dzib… - Astronomy & …, 2021 - aanda.org
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 …

Core-collapse supernovae in dense environments–particle acceleration and non-thermal emission

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 …

Morphology of supernova remnants and their halos

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 …

Spectral softening in core-collapse supernova remnant expanding inside wind-blown bubble

S Das, R Brose, DMA Meyer, M Pohl, I Sushch… - Astronomy & …, 2022 - aanda.org
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 …

Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

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 …