|
ИСТИНА |
Войти в систему Регистрация |
ИСТИНА ИНХС РАН |
||
The very high energy characteristics of shell-type SNRs and Pulsar Wind Nebulae at different agesстатья
- Авторы: Sinitsyna V.G., Alaverdyan A.Y., Andreeva M.S., Balygin K.A., SBorisov S., Ivanov I.A., Kirichenko A.M., Klimov A.I., Kozhukhova I.P., Mirzafatikhov R.M., Moseiko N.I., Nikolsky S.I., Ostashev I.E., IPalamarchuk A., Sinitsyna V.Y., Volokh I.G.
- Журнал: Journal of Physics: Conference Series
- Том: 718
- Год издания: 2016
- Издательство: IOP Publishing
- Местоположение издательства: [Bristol, UK], England
- DOI: 10.1088/1742-6596/718/5/052045
- Аннотация: The investigation of VHE gamma-ray sources by any methods, including mirror Cherenkov telescopes, touches on the problem of the cosmic ray origin and, accordingly, the role of the Galaxy in their generation. The SHALON observations have yielded the results on Galactic supernova remnants of shell-type and Pulsar Wind Nebulae of different ages. For each of SNRs the observation results are presented with spectral energy distribution by SHALON in comparison with other experiment data and images by SHALON. The data obtained suggest that the very high energy γ-ray emission in the objects being discussed is different in origin
- Добавил в систему: Андреева Мария Сергеевна