Saz Parkinson, P. M. (2011) Gamma-ray pulsars in the Fermi LAT era. Il nuovo cimento C, 34 (3). pp. 173-178. ISSN 1826-9885
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Abstract
Observations over the past two years with the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope have led to a tenfold increase in the number of known γ-ray pulsars. Roughly one third of this population consists of young radio-loud pulsars, one third are radio-quiet pulsars discovered in blind searches of LAT data, and one third are γ-ray millisecond pulsars (MSPs). In this paper I discuss what we have learned about these three populations, as well as prospects for further discoveries.
| Item Type: | Article |
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| Uncontrolled Keywords: | γ-ray ; Pulsars |
| Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
| Depositing User: | Marina Spanti |
| Date Deposited: | 06 Apr 2020 18:34 |
| Last Modified: | 06 Apr 2020 18:34 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/17263 |
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