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Observations of the Li, Be, and B isotopes and constraints on cosmic-ray propagation
G. A. de Nolfo, I. V. Moskalenko, W. R. Binns +14
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCR) between E=50-200 MeV/nucleon has been observed by the Cosmic Ray Isotope Spectrometer (CRIS) on NASA's ACE mis…
Source population synthesis and the Galactic diffuse gamma-ray emission
A. W. Strong
Population synthesis is used to study the contribution from undetected sources to the Galactic ridge emission measured by EGRET. Synthesized source counts are compared with the 3rd…
Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
Troy A. Porter, Igor V. Moskalenko, Andrew W. Strong
The evidence for particle acceleration in supernova shells comes from electrons whose synchrotron emission is observed in radio and X-rays. Recent observations by the HESS instrume…
Gamma-rays from halos around stars and the Sun
Elena Orlando, Andrew Strong
Inverse Compton scattering by relativistic electrons produces a major component of the diffuse emission from the Galaxy. The photon fields involved are the cosmic microwave backgro…