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

dc.contributor.author	Sushchov, O.B.
dc.contributor.author	Kobzar, O.O.
dc.contributor.author	Hnatyk, B.I.
dc.contributor.author	Marchenko, V.V.
dc.date.accessioned	2017-06-04T18:41:02Z
dc.date.available	2017-06-04T18:41:02Z
dc.date.issued	2012
dc.identifier.citation	Centaurus 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.issn	2227-1481
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/119177
dc.description.abstract	For 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.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	Centaurus A as a plausible source of ultra high energy cosmic rays registered by the Pierre Auger Observatory	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA