Cosmic rays from supernova remnants and superbubbles
arXiv:1807.09726 · doi:10.1016/j.asr.2017.04.006
Abstract
Recent high energy gamma-ray observations of both single supernova remnants and superbubbles, together with observations of supernovae, star formation regions, and local cosmic ray composition, now provide an integrated framework tying together the sources, injection, acceleration and propagation of the cosmic rays, so that it is possible to determine their relative contributions to cosmic ray acceleration for all but the very highest energies.
24 pages, 8 figures
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Cited by in corpus (15)
- Impact of low-energy cosmic rays on star formation
- High-energy particles and radiation in star-forming regions
- Cosmic ray production in supernovae
- Cosmic ray production in superbubbles
- Cosmic-Ray Diffusion Suppression in Star-forming Regions Inhibits Clump Formation in Gas-rich Galaxies
- Massive star cluster origin for the galactic cosmic ray population at very-high energies
- Low energy cosmic rays
- Shocks and non-thermal particles in clusters of galaxies
- The Origin of Cosmic Rays: How Their Composition Defines Their Sources and Sites, and the Processes of Their Mixing, Injection and Acceleration
- Modeling of GeV-TeV gamma-ray emission of Cygnus Cocoon
- The cosmic-ray content of the Orion-Eridanus superbubble
- High-energy cosmic rays from compact galactic star clusters: particle fluxes and anisotropy
- Wolf-Rayet stars in young massive star clusters as potential sources of Galactic cosmic rays
- Supernova remnants in super bubbles as cosmic ray accelerators
- Can superbubbles accelerate ultra-high energy protons?