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A Survey of General Relativistic Magnetohydrodynamic Models for Black Hole Accretion Systems

  • Authors: Vedant Dhruv, Cora Prather, George N. Wong, Charles F. Gammie

Vedant Dhruv et al 2025 The Astrophysical Journal Supplement Series 277 .

  • Provider: AAS Journals

Caption: Figure 9.

Time- and azimuth-averaged “jet profiles” (σ = 1 contours). The solid (dashed) lines represent MAD (SANE) models. The filled gray circle at the lower-left corner denotes a zero spin black hole (reh = 2 rg).

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