|
ИСТИНА |
Войти в систему Регистрация |
Интеллектуальная Система Тематического Исследования НАукометрических данных |
||
Very high energy emission sources beyond the Galaxyстатья
- Авторы: Sinitsyna V.G., Andreeva M.S., Balygin K.A., Borisov S.S., Ivanov I.A., Kirichenko A.M., Klimov A.I., Kozhukhova I.P., Mirzafatikho R.M., Moseiko N.I., Ostashev I.E., Palamarchuk A.I., Sinitsyna V.Y., Volokh and I.G
- Сборник: EPJ Web of Conferences
- Серия: Proceedings of the XXIII International Workshop “High Energy Physics and Quantum Field Theory” (QFTHEP 2017)
- Том: 145
- Год издания: 2017
- Место издания: EPJ Web of Conferences
- DOI: 10.1051/epjconf/201714519004
- Аннотация: Active Galactic Nuclei (AGN) are considered as potential extragalactic sources of very and ultra high energy cosmic rays. According to theoretical predictions cosmic ray acceleration can take place at the shock created by the expanding cocoons around active galactic nuclei as well as at AGN jets. The measurements of AGN TeV spectra, the variability time scale of TeV emission can provide essential information on the dynamics of AGN jets, the localization of acceleration region and an estimation of its size. SHALON observations yielded data on extragalactic sources of different AGN types in the energy range of 800GeV–100TeV. The data from SHALON observations are compared with those from other experiments at high and very high energies.
- Добавил в систему: Андреева Мария Сергеевна