Input of nearby sources in spectra and anisotropy of ultrahigh energy cosmic rays
- Authors: Zirakashvili V.N.1, Ptuskin V.S.1, Rogovaya S.I.1
- 
							Affiliations: 
							- Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation of the Russian Academy of Sciences
 
- Issue: Vol 87, No 7 (2023)
- Pages: 951-953
- Section: Articles
- URL: https://rjpbr.com/0367-6765/article/view/654345
- DOI: https://doi.org/10.31857/S0367676523701661
- EDN: https://elibrary.ru/ONXZRC
- ID: 654345
Cite item
Abstract
Propagation of ultrahigh energy cosmic rays from nearby sources was investigated. It is shown that observable spectrum, chemical composition and anisotropy at energies above 5 · 1018 eV can be explained in the model of one nearby source galaxy M87 with heavy chemical composition.
About the authors
V. N. Zirakashvili
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagationof the Russian Academy of Sciences
							Author for correspondence.
							Email: zirak@izmiran.ru
				                					                																			                												                								Russia, 108840, Moscow						
V. S. Ptuskin
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagationof the Russian Academy of Sciences
														Email: zirak@izmiran.ru
				                					                																			                												                								Russia, 108840, Moscow						
S. I. Rogovaya
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagationof the Russian Academy of Sciences
														Email: zirak@izmiran.ru
				                					                																			                												                								Russia, 108840, Moscow						
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