Image Details

Choose export citation format:

Slow Cosmic-Ray Diffusion in Supersonic and Super-Alfvénic Turbulence

  • Authors: Yue Hu

Yue Hu 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 5.

Physical diffusion coefficients for Ms ≃ 10 turbulence, adopting Lbox = 1 pc. The left and right panels show MA ≃ 5 and MA ≃ 10, respectively. Solid and dashed curves denote D and D; blue and red denote solenoidal and compressive forcing. Shaded bands indicate representative diffusion ranges inferred for the Cygnus Bubble, the Geminga halo, and the V4641 Sgr microquasar.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse