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Oblique Shocks at Supernova Remnants in Massive Star Clusters: A Model for the Cosmic-Ray Knee Observed by LHAASO

  • Authors: Luana N. Padilha, R. C. Dos Anjos

Luana N. Padilha and R. C. Dos Anjos 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 6.

CR composition in terms of the mean logarithmic atomic mass 〈ln A〉, derived from Models A, B, and C and compared with data from AUGER (A. Yushkov 2019; B. Pont 2023), TALE (R. U. Abbasi et al. 2021), TUNKA (P. A. Bezyazeekov et al. 2018; N. M. Budnev et al. 2022), IceTop (IceCube Collaboration et al. 2013), KASCADE (L. G. Sveshnikova et al. 2013), JACEE (Y. Takahashi et al. 1998), and ATIC (A. D. Panov et al. 2009).

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