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Young and Millisecond Pulsar GeV Gamma-ray Fluxes from the Galactic Center and Beyond
- Source :
- NASA Astrophysics Data System
- Publication Year :
- 2016
-
Abstract
- Gamma-ray observations have shown pulsars to be efficient converters of rotational energy into GeV photons and it is of wide-ranging interest to determine their contribution to the gamma-ray background. We arrive at flux predictions from both the young (<br />Comment: Submitted to Phys. Rev. D
- Subjects :
- High Energy Astrophysical Phenomena (astro-ph.HE)
High Energy Physics - Phenomenology
High Energy Physics - Phenomenology (hep-ph)
Astrophysics of Galaxies (astro-ph.GA)
Astrophysics::High Energy Astrophysical Phenomena
Astrophysics::Instrumentation and Methods for Astrophysics
FOS: Physical sciences
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics - High Energy Astrophysical Phenomena
Astrophysics - Astrophysics of Galaxies
Astrophysics::Galaxy Astrophysics
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- NASA Astrophysics Data System
- Accession number :
- edsair.doi.dedup.....92c0b0c9a8a666b739bc7a75d794ca63