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Acceleration and propagation of ultra high energy cosmic rays in the Local Universe
ПРИСКОРЕННЯ ТА ПОШИРЕННЯ КОСМІЧНИХ ПРОМЕНІВ НАДВИСОКИХ ЕНЕРГІЙ У ЛОКАЛЬНОМУ ВСЕСВІТІ
2018
Bulletin of Taras Shevchenko National University of Kyiv Astronomy
ПРИСКОРЕННЯ ТА ПОШИРЕННЯ КОСМІЧНИХ ПРОМЕНІВ НАДВИСОКИХ ЕНЕРГІЙ У ЛОКАЛЬНОМУ ВСЕСВІТІ
Distribution of matter in the Local Universe (up to ~ 100 Mpc), especially in a Virgo Supercluster region (~20 Mpc) is strongly nonuniform and includes all elements of large scale structure: galaxies and their clusters, superclusters, filaments, sheets and voids. On its smallest scale, our Galaxy and its similar galaxy M31 (Andromeda Nebula) at a distance 770 kpc, together with dozens of dwarf galaxies, form the Local Group of Galaxies. Local group contained in Local Sheet – suchlike pancake
doi:10.17721/btsnua.2018.58.33-36
fatcat:wf54i2e2yvfbrj23nekpcek43i