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Search for sources of primary cosmic rays at energy above 0.1 PeV at the Tien Shan

✍ Scribed by G. Benkó; A.P. Chubenko; G. Erdös; S.I. Nikolsky; N.M. Nesterova; V.A. Romakhin; A.L. Shchepetov; A. Somogy; A. Varga

Publisher: Elsevier Science
Year: 2008
Tongue: English
Weight: 164 KB
Volume: 175-176
Category: Article
ISSN: 0920-5632
DOI: 10.1016/j.nuclphysbps.2007.11.066

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✦ Synopsis

Analysis of the experimental data of joint Russian -Hungarian (FIAN and KFKI) research was carried out at Tien Shan station for the search of sources of primary cosmic rays (PCR) at energies (E0 = 10 14 -10 15 eV). Maps of extensive air shower (EAS) arrival directions are presented where the standard deviation of mean event numbers in equatorial coordinates exceeded a definite value. The excess of EAS number was observed from some directions. It was observed from an extended galactic object -the SN remnant. The young pulsar PSR 0656+14 is located near the centre of this object.

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