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A method to constrain the characteristic angular size of the brightest cosmic-ray sources observed above 57 × 10<sup>18</sup> eV

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

Younk, P. W.
  • 期刊名称Astrophysics and Space Sciences Transactions
  • 作者Younk, P. W.
  • 卷第7卷
  • 期第3期
  • 电子ISSN1810-6536
  • 文件大小368.35KB
  • 发表时间2011-09-20
  • DOI10.5194/astra-7-403-2011
  • 页码403-410
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