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The Pierre Auger Collaboration has provided a compelling indication for apossible correlation between the arrival directions of ultrahigh-energy cosmicrays and nearby starburst galaxies. Herein we show how the latest large-scalemodeling of starburst galaxies is compatible with the cosmic rays producing theanisotropy signal being accelerated at the terminal shock of superwinds.

Exploring the superwind mechanism for generating ultrahigh-energy cosmic rays using large-scale modeling of starbursts