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Cosmic-Ray and Plasma Coupling for Isothermal Supersonic Turbulence in the Magnetized Interstellar Medium

  • Authors: Matt L. Sampson, James R. Beattie, Romain Teyssier, Philipp Kempski, Eric R. Moseley, Benoit Commerçon, Yohan Dubois, Joakim Rosdahl

Matt L. Sampson et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 6.

The same as Figure 5 except for the two-dimensional probability density function of the CR flux magnitude ∥Fc∥ and ρ. In the strong coupling regime (top right panels), we observe ∥Fc∥ ∝ ρ4/3 (see Equation (19)).

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