activity
19942005
most citedHydrodynamic Turbulence in Accretion Disks

2 citations · 2 across the 3 of their papers we have counts for

collaborators

13 papers

astro-ph20052 cited

Hydrodynamic Turbulence in Accretion Disks

Banibrata Mukhopadhyay, Niayesh Afshordi, Ramesh Narayan

Turbulent viscosity in cold accretion disks is likely to be hydrodynamic in origin. We investigate the growth of hydrodynamic perturbations in a small region of a disk, which we mo…

astro-ph2003

Evidence for the Black Hole Event Horizon

Ramesh Narayan

Astronomers have discovered many candidate black holes in X-ray binaries and in the nuclei of galaxies. The candidate objects are too massive to be neutron stars, and for this reas…

astro-ph2002

On the Minimum Energy Configuration of a Rotating Barotropic Fluid

Ramesh Narayan, James E. Pringle

In a recent paper (astro-ph/0207561, posted on July 25, 2002), Fromang & Balbus state that ``a uniformly rotating barotropic fluid in an external potential attains a true energy mi…

astro-ph2001

Thermal Conduction and the Stability of Hot Accretion Flows

Mikhail V. Medvedev, Ramesh Narayan

Recently, Medvedev & Narayan (2001) discovered a new type of accretion flow, a hot settling flow around a rapidly rotating neutron star. The flow is cooling-dominated and energetic…

gr-qc1998

Astrophysical Evidence for Black Hole Event Horizons

Kristen Menou, Eliot Quataert, Ramesh Narayan

Astronomers have discovered many potential black holes in X-ray binaries and galactic nuclei. These black holes are usually identified by the fact that they are too massive to be n…

astro-ph1998

Advection-Dominated Accretion around Black Holes

Ramesh Narayan, Rohan Mahadevan, Eliot Quataert

This article reviews the physics of advection-dominated accretion flows (ADAFs) and describes applications to several black hole X-ray binaries and galactic nuclei. The possibility…