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handle: 11568/158767
The Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope provides both direct and indirect measurements of Galactic cosmic rays (CR). The LAT high-statistics observations of the 7 GeV - 1 TeV electron plus positron spectrum and limits on spatial anisotropy constrain models for this cosmic-ray component. On a Galactic scale, the LAT observations indicate that cosmic- ray sources may be more plentiful in the outer Galaxy than expected or that the scale height of the cosmic-ray diffusive halo is larger than conventional models. Production of cosmic rays in supernova remnants (SNR) is supported by the LAT gamma-ray studies of several of these, both young SNR and those interacting with molecular clouds.
20 pages, 12 figures, to be published in Astroparticle Physics
High Energy Astrophysical Phenomena (astro-ph.HE), Astronomy, Cosmic rays; Gamma rays; Observations, FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena, Astro
High Energy Astrophysical Phenomena (astro-ph.HE), Astronomy, Cosmic rays; Gamma rays; Observations, FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena, Astro
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 21 | |
popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 10% | |
influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 10% | |
impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Top 10% |