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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 2.

Spatial distribution of MSCs in the Galactic plane. Top panel: combined sample that includes the simulated population and the observed objects, projected onto the X-Y plane. The green circle marks the sources inside a radius of 3.0 kpc from the Sun as listed by N. V. Kharchenko et al. (2013). Bottom panel: the observational catalog alone with the same projection. Gray curves indicate the spiral pattern adopted for visual reference.

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