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NuSTAR Hard X-Ray Spectra of Radio Galaxies

  • Authors: Jialai Kang, Junxian Wang, and Wenyong Kang

2020 The Astrophysical Journal 901 111.

  • Provider: AAS Journals

Caption: Figure 9.

The Γ vs. reflection factor R of our sample and PW19. The green line shows the expected R vs. Γ curve based on the model in Beloborodov (1999), which is a result of the relative motion of the outflowing corona with respect to the disk.

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