Image Details

Choose export citation format:

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 19.

A poloidal cut of an MAD simulation illustrating various definitions of a jet or outflow. The background color saturation represents rest-mass density in code units. The gold lines mark geometric boundaries at θ = 1 and θ = π − 1, which are used in this work to compute the total outflow power Pout. The blue line is the −ut = 1 contour, while the magenta line represents βγ = 1, the latter serving as the jet definition in this study. The green, plum, and red lines indicate contours where μ = 1, Be = 1 (fluid Bernoulli parameter), and σ = 1, respectively.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse