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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 1.

The 3D distribution of the selected MSCs from the N. V. Kharchenko et al. (2013) catalog in Sun-centered Cartesian coordinates (X, Y, Z in kpc). Marker color encodes the cluster age, and larger markers indicate higher estimated cluster mass M cl (selection requires M cl > 103 M ); the concentration near Z ≃ 0 traces the Galactic midplane.

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