Razzano, Massimiliano (2011) The gamma-ray pulsar in the Gamma Cygni supernova remnant. Il nuovo cimento C, 34 (3). pp. 179-182. ISSN 1826-9885
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Abstract
We report updated results on PSR J2021+4026, based on the latest data collected by the Fermi Large Area Telescope. This pulsar was discovered using blind search techniques in the error box of the EGRET source 3EG J2020+4017 in the Gamma Cygni supernova remnant (SNR G78.2+2.1). This source is located in a quite complex region, mainly because of the highly structured diffuse Galactic background. Since its discovery in gamma rays no other pulsed counterparts for PSR J2021+4026 have been found at other wavelengths (e.g., radio), and this could put important constraints on its emission characteristics. We present recent results of the analysis of the gamma-ray emission from this pulsar, including spatial analysis, as well as of the temporal and spectral analysis of this source.
| 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 18:35 |
| Last Modified: | 06 Apr 2020 18:35 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/17264 |
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