Search for Sources of Primary Cosmic Rays at Energies Above 0.1 Pev at Tien Shan

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dc.creatorBenko, G.
dc.creatorErdos, G.
dc.creatorNikolsky, S. I.
dc.creatorNesterova, N. M.
dc.creatorRomakhin, V. A.
dc.creatorChubenko, A. P.
dc.creatorShepetov, A. L.
dc.creatorSomogyi, A.
dc.creatorVarga, A.
dc.date2005-02-03
dc.date2005-02-25
dc.date.accessioned2026-07-07T02:16:55Z
dc.date.available2026-07-07T02:16:55Z
dc.descriptionAnalysis of the experimental data of joint Russian - Hungarian research was carried out at Tien Shan station on the search of sources of primary cosmic rays (PCR) at energies 0.1-1.0 PeV. Maps of extensive air shower arrival directions were presented where the standard deviation of mean event numbers in equatorial co-ordinates exceeded a definite value. The excess of EAS number was observed from an Galaxy object - the SN remnant and some other directions. The young pulsar PSR 0656+14 located near the centre of this object.
dc.description4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0502065
dc.identifierhttp://arxiv.org/abs/astro-ph/0502065
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8979
dc.subjectAstrophysics
dc.titleSearch for Sources of Primary Cosmic Rays at Energies Above 0.1 Pev at Tien Shan
dc.typetext

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