The dynamical structure of nonradiative black hole accretion flows

We analyze three-dimensional magnetohydrodynamic 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 generated se...

Szczegółowa specyfikacja

Opis bibliograficzny
Główni autorzy: Hawley, J, Balbus, SA
Format: Journal article
Język:English
Wydane: Institute of Physics Publishing 2002