Gamma rays from Galactic Pulsars
| Authors |
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|---|---|
| Publication date | 2015 |
| Journal | Nuclear and Particle Physics Proceedings |
| Event | Neutrino Oscillation Workshop (NOW 2014) |
| Volume | Issue number | 265-266 |
| Pages (from-to) | 236-238 |
| Organisations |
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| Abstract | Gamma rays from young pulsars and milli-second pulsars are expected to contribute to the diuse gamma-ray emission measured by the Fermi Large Area Telescope (LAT) at high latitudes. We derive the contribution of the pulsars undetected counterpart by using information from radio to gamma rays and we show that they explain only a small fraction of the isotropic diuse gamma-ray background. |
| Document type | Article |
| Note |
Proceedings title: Proceedings of the Neutrino Oscillation Workshop (NOW 2014) : Conca Specchiulla, Otranto, Lecce, Italy, September 7-14, 2014 Publisher: Elsevier Place of publication: Amsterdam Editors: P. Bernardini, G. Fogli, E. Lisi |
| Language | English |
| Published at |
https://doi.org/10.1016/j.nuclphysbps.2015.06.060
(Final published version)
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