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Search for the astrophysical sources of the Fly's Eye event with the highest to date cosmic ray energy E=3.2·10²⁰ eV

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dc.contributor.author Gnatyk, R.B.
dc.contributor.author Kudrya, Yu.N.
dc.contributor.author Zhdanov, V.I.
dc.date.accessioned 2017-06-10T13:15:45Z
dc.date.available 2017-06-10T13:15:45Z
dc.date.issued 2016
dc.identifier.citation Search for the astrophysical sources of the Fly's Eye event with the highest to date cosmic ray energy E=3.2·10²⁰ eV / R.B. Gnatyk, Yu.N. Kudrya, V.I. Zhdanov // Advances in Astronomy and Space Physics. — 2016. — Т. 6., вип. 1. — С. 41-44. — Бібліогр.: 25 назв. — англ. uk_UA
dc.identifier.issn 2227-1481
dc.identifier.other DOI:10.17721/2227-1481.6.41-44
dc.identifier.uri http://dspace.nbuv.gov.ua/handle/123456789/119949
dc.description.abstract Among the registered extremely high energy cosmic rays (EHECR, E > 10²⁰ eV) an event with the highest to date energy of E = 3.2 · 10²⁰ eV was detected by the Fly's Eye experiment (FE event) in 1991. With the use of the back-tracking method for the calculation of the EHECR trajectories in Galactic and extragalactic magnetic fields, we show that the galaxies UGC 03574 and UGC 03394 are the most promising candidates among the nearby extragalactic sources for the cases of iron and C-N-O group primary nucleus respectively. The most likely accelerating mechanisms are the newly-born millisecond pulsars, magnetar ares and tidal disruption events in these galaxies. uk_UA
dc.description.sponsorship The data in Table 1 are taken from the NASA/IPAC Extragalactic Database. This publication is based on the research supported by the grant of the State Fund For Fundamental Research of Ukraine (project F64/42-2016). uk_UA
dc.language.iso en uk_UA
dc.publisher Головна астрономічна обсерваторія НАН України uk_UA
dc.relation.ispartof Advances in Astronomy and Space Physics
dc.title Search for the astrophysical sources of the Fly's Eye event with the highest to date cosmic ray energy E=3.2·10²⁰ eV uk_UA
dc.type Article uk_UA
dc.status published earlier uk_UA


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