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pro vyhledávání: '"Vera G. Sinitsyna"'
Autor:
Vera G. Sinitsyna, Vera Y. Sinitsyna
Publikováno v:
Universe, Vol 9, Iss 2, p 98 (2023)
Supernova Remnants (SNRs) are generally believed to produce the cosmic rays in our Galaxy due to the powerful supernova blast waves generated by expanding SNRs. In contrast to the leptonic cosmic-ray component that is clearly seen by the SNR emission
Externí odkaz:
https://doaj.org/article/9046c085fe764292afde90779a4dd7ff
Autor:
Vera G. Sinitsyna, Vera Yu. Sinitsyna
Publikováno v:
Universe, Vol 8, Iss 2, p 57 (2022)
Cyg X-3 is the famous binary system containing a black hole that is actively studied through a wide range of the electromagnetic spectrum, from radio wavelengths to ultra-high-energy gamma-rays, but still not well-understood. The Cyg X-3 focusing inv
Externí odkaz:
https://doaj.org/article/9a6c8f8e472340c481be93d63b891b53
Autor:
Vera G. Sinitsyna, Vera Y. Sinitsyna
Publikováno v:
Astronomische Nachrichten. 344
Publikováno v:
Astronomische Nachrichten. 344
Autor:
Vera G. Sinitsyna, Vera Yu. Sinitsyna, Sergei S. Borisov, Rim M. Mirzafatikhov, Kirill A. Balygin, Anatolii I. Klimov, Igor E. Ostashev, Nikolai I. Moseiko
Publikováno v:
Astronomische Nachrichten. 344
Autor:
Vera G. Sinitsyna, Vera Y. Sinitsyna
Publikováno v:
Astronomische Nachrichten. 344
Publikováno v:
EPJ Web of Conferences. 260:11033
The Pamela, Fermi, AMS-02 spectrometer experimental data cannot be explained using the diffusive models of propagation of cosmic-rays accelerated at the supernova shocks and require the existence of nearby sources of cosmic rays at the distances less
Autor:
Vera G. Sinitsyna, Vera Y. Sinitsyna
Publikováno v:
EPJ Web of Conferences. 260:11050
The overall observations of plerions from radio to the very high energy gamma-rays could provide information about the evolution of PWN from the young Crab-like to the older stages. The extended MeV-TeV emission from Geminga middle-aged pulsar of ~ 3
Autor:
Vera Yu. Sinitsyna, Vera G. Sinitsyna
Publikováno v:
EPJ Web of Conferences. 260:11047
OJ 287 is one of the most studied BL Lacs with very long optical measurements which spectrum has been well measured through radio to X-rays. OJ 287 is supposed to be a binary black hole system. Its secondary black hole passes the accretion disk of th