Search for Sources of Ultrahigh Energy Cosmic Rays
| dc.creator | Mikhailov, A. A. | |
| dc.date | 1999-06-18 | |
| dc.date.accessioned | 2026-07-07T02:32:05Z | |
| dc.date.available | 2026-07-07T02:32:05Z | |
| dc.description | The connection between the arrival directions of ultrahigh energy cosmic rays by using the EAS array data and point galactic sources of radio-and gamma-radiations, pulsars,is sought. At the mean particle energy of 10^{19} eV the correlation between the particle arrival directions and pulsars located along the magnetic field lines has been found. According to our estimations the chance probability is equal to 2.10^{-4}. The observed particle flux from 16 pulsars inside a circle of radius <6^{\circ} exceeds the background by 6.3σ(p < 10^{-10}), from PSR 2351+61 - 5σ. A group of 9 pulsars has been found from the direction of which the particle flux in the region 10^{\circ}\times60^{\circ} is in excess of the expected one by 4.4σ. The obtained results are discussed. | |
| dc.description | 4 pages,7 figures,to appear in Proceedings of 26th ICRC(Salt Lake City), OG 1.3.08 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9906302 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9906302 | |
| dc.identifier | Proceedings 26-th ICRC(Salt Lake City),1999,v.3,p.268. | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14383 | |
| dc.subject | Astrophysics | |
| dc.title | Search for Sources of Ultrahigh Energy Cosmic Rays | |
| dc.type | text |