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

dc.contributor.author	Kobzar, O.
dc.contributor.author	Hnatyk, B.
dc.contributor.author	Marchenko, V.
dc.contributor.author	Bogdan, T.
dc.date.accessioned	2017-06-02T18:35:38Z
dc.date.available	2017-06-02T18:35:38Z
dc.date.issued	2011
dc.identifier.citation	Propagation 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.isbn	987-966-439-367-3
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/118983
dc.description.abstract	Propagation 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.language.iso	en	uk_UA
dc.publisher	Advances in astronomy and space physics	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.title	Propagation of different components of cosmic rays from Centaurus A in the Galactic magnetic fields	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA