Propagation of different components of cosmic rays from Centaurus A in the Galactic magnetic fields

dc.contributor.authorKobzar, O.
dc.contributor.authorHnatyk, B.
dc.contributor.authorMarchenko, V.
dc.contributor.authorBogdan, T.
dc.date.accessioned2017-06-02T18:35:38Z
dc.date.available2017-06-02T18:35:38Z
dc.date.issued2011
dc.description.abstractPropagation of different chemical composition ultrahigh energy cosmic rays in the galactic magnetic fields was simulated. The simulation for the ultra high energy events, registered by the AUGER observatory in the sky region near Centaurus A was performed. It is shown that some of these events could originate from Centaurus A.uk_UA
dc.identifier.citationPropagation of different components of cosmic rays from Centaurus A in the Galactic magnetic fields / O. Kobzar, B. Hnatyk, V. Marchenko, T. Bogdan // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 47-49. — Бібліогр.: 5 назв. — англ.uk_UA
dc.identifier.isbn987-966-439-367-3
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/118983
dc.language.isoenuk_UA
dc.publisherAdvances in astronomy and space physicsuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titlePropagation of different components of cosmic rays from Centaurus A in the Galactic magnetic fieldsuk_UA
dc.typeArticleuk_UA

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