| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1771136 | Astroparticle Physics | 2011 | 9 Pages |
Abstract
⺠Ultrahigh energy heavy nuclei deflected in the Galactic magnetic field. ⺠Both regular and turbulent Galactic magnetic field components are modeled. ⺠Turbulent field impact on source images at low and high Galactic latitudes. ⺠Strong source fluxes (de)magnifications reduced by the turbulent field. ⺠Cen A cannot be the sole source of all UHECR detected at Earth above 55 EeV.
Keywords
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Astronomy and Astrophysics
Authors
G. Giacinti, M. KachelrieÃ, D.V. Semikoz, G. Sigl,