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pro vyhledávání: '"Shibanov, Yuri A."'
The young radio pulsar J1124-5916 is associated with a Cas A like supernova remnant G292.0+1.8. It powers a compact torus-like pulsar wind nebula with a jet first detected in X-rays and then identified in the optical and mid-infrared. We carried out
Externí odkaz:
http://arxiv.org/abs/1304.8105
Publikováno v:
MNRAS, 2011, Volume 415, pp. 867--880
The Vela and Geminga pulsars are rotation powered neutron stars, which have been identified in various spectral domains, from the near-infrared to hard $\gamma$-rays. In the near-infrared they exhibit tentative emission excesses, as compared to the o
Externí odkaz:
http://arxiv.org/abs/1103.4871
We have performed a deep optical imaging of 3C 58 SNR with the NOT in the B and V bands to detect the optical counterpart of the associated pulsar J0295+6449 and its torus-like wind nebula visible in X-rays. We analyzed our data together with the arc
Externí odkaz:
http://arxiv.org/abs/0802.2386
Autor:
Shibanov, Yuri A., Zharikov, Sergei V., Komarova, Viktoria N., Kawai, Nobuyuki, Urata, Yuji, Koptsevich, Alexey B., Sokolov, Vladimir V., Shibata, Shinpei, Shibazaki, Noriaki
We carried out a deep subarcsecond BRI imaging of the two middle-aged pulsars to establish their properties in the optical range. Both pulsars are detected at >10 sigma level. Geminga is for the first time reliably detected in the I band with a magni
Externí odkaz:
http://arxiv.org/abs/astro-ph/0511311
Autor:
Shibanov, Yuri S.
Publikováno v:
Leonardo, 1989 Jan 01. 22(1), 49-54.
Externí odkaz:
https://www.jstor.org/stable/1575139
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