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CHANG-ES. XXXVIII. A Thin Radio Halo Shaped by Slow Cosmic-Ray Transport in the Quiescent Galaxy NGC 4565

  • Authors: Jianghui Xu, Jiang-Tao Li, Guilin Liu, Luan Luan, Volker Heesen, Rainer Beck, Judith Irwin, Q. Daniel Wang, Michael Stein, Li-Yuan Lu, Yang Yang, Jeroen Stil, Jayanne English, Ralf-Jürgen Dettmar

Jianghui Xu et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 5.

Vertical profiles of the nonthermal radio continuum emission at the S-band. The top-center panel shows the locations of the five analysis strips (E2, E1, C, W1, and W2) overlaid on the nonthermal intensity map. The other five panels display the corresponding vertical profile for each strip, arranged symmetrically around the setup panel. In each profile panel, the black points represent the measured flux density, averaged within 6″ × 120″ (0.35 × 6.92 kpc) boxes. Positive distances are to the north of the major axis, and negative distances are to the south. The red curve is the best-fit two-component Gaussian profile.

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