Astrophys. Space Sci. Trans., 7, 403-410, 2011
www.astrophys-space-sci-trans.net/7/403/2011/
doi:10.5194/astra-7-403-2011
© Author(s) 2011. This work is distributed
under the Creative Commons Attribution 3.0 License.
 
20 Sep 2011


A method to constrain the characteristic angular size of the brightest cosmic-ray sources observed above 57 × 1018 eV

P. W. Younk

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