The Dynamical Structure of Nonradiative Black Hole Accretion Flows
We analyze three-dimensional magnetohydrodynamic (MHD) simulations of a nonradiative accretion flow around a black hole using a pseudo-Newtonian potential. The flow originates from a torus initially centered at 100 gravitational (Schwarzschild) radii. Accretion is driven by turbulent stresses genera...
| প্রধান লেখক: | , |
|---|---|
| বিন্যাস: | Journal article |
| প্রকাশিত: |
2002
|