Centaurus A as a plausible source of ultra high energy cosmic rays registered by the Pierre Auger Observatory

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dc.contributor.authorSushchov, O.B.
dc.contributor.authorKobzar, O.O.
dc.contributor.authorHnatyk, B.I.
dc.contributor.authorMarchenko, V.V.
dc.date.accessioned2017-06-04T18:41:02Z
dc.date.available2017-06-04T18:41:02Z
dc.date.issued2012
dc.description.abstractFor ultra high energy cosmic rays events detected by the Pierre Auger Observatory which arrive from the region near Centaurus A the positions of the corresponding sources were calculated for the two chosen galactic magnetic field models. Also the influence of extragalactic magnetic field was taken into account for different energy and ultra high energy cosmic rays type to show the possibility of correlation with Centaurus A.uk_UA
dc.identifier.citationCentaurus A as a plausible source of ultra high energy cosmic rays registered by the Pierre Auger Observatory / O.B. Sushchov, O.O. Kobzar, B.I. Hnatyk, V.V. Marchenko // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 73-75. — Бібліогр.: 7 назв. — англ.uk_UA
dc.identifier.issn2227-1481
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/119177
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleCentaurus A as a plausible source of ultra high energy cosmic rays registered by the Pierre Auger Observatoryuk_UA
dc.typeArticleuk_UA

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Advances in Astronomy and Space Physics, 2012, вип. 1