Magnetar SGR 1900+14 as a Potential Source of Galactic Cosmic Rays with Energies Above 1020 eV
Author:
Publisher
Allerton Press
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.3103/S0884591318040037.pdf
Reference21 articles.
1. R. Gnatyk and V. Zhdanov, “Search of the Galactic sources of the cosmic ray triplet with energies above 1020 eV” Bulletin of National Taras Shevchenko University of Kyiv. Astronomy. 53 (1), 37–40 (2016).
2. A. Aab, P. Abreu, M. Aglietta, et al., “Searches for large-scale anisotropy in the arrival directions of cosmic rays detected above energy of 1019 eV at the Pierre Auger Observatory and the Telescope Array,” Astrophys. J. 794, 172 (2014).
3. A. Aab, P. Abreu, M. Aglietta, et al., “Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory,” Astrophys. J. 804, 15 (2015).
4. A. U. Abeysekara, A. Albert, R. Alfaro, et al., “The 2HWC HAWC Observatory Gamma Ray Catalog,” Astrophys. J. 843, 40 (2017).
5. F. A. Aharonian, Very High Energy Cosmic Gamma Radiation: A Crucial Window on the Extreme Universe (World Sci., Singapore, 2004), p. 495.
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1. Unveiling the nature of the unidentified gamma-ray sources 4FGL J1908.6+0915e, HESS J1907+089/HOTS J1907+091, and 3HWC J1907+085 in the sky region of the magnetar SGR 1900+14;Monthly Notices of the Royal Astronomical Society;2022-05-11
2. High-energy gamma-ray emission from SNR G57.2+0.8 hosting SGR J1935+2154;Journal of Cosmology and Astroparticle Physics;2021-10-01
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