activity
20052010
most citedThe Spin of the Near-Extreme Kerr Black Hole GRS 1915+105

586 citations · 1.6k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2010★ 310 cited

Simulations of Magnetized Disks Around Black Holes: Effects of Black Hole Spin, Disk Thickness, and Magnetic Field Geometry

Robert F. Penna, Jonathan C. McKinney, Ramesh Narayan +3

The standard general relativistic model of a razor-thin accretion disk around a black hole, developed by Novikov & Thorne (NT) in 1973, assumes the shear stress vanishes at the rad…

astro-ph2008★ 184 cited

Three-Dimensional Simulations of Magnetized Thin Accretion Disks around Black Holes: Stress in the Plunging Region

Rebecca Shafee, Jonathan C. McKinney, Ramesh Narayan +3

We describe three-dimensional general relativistic magnetohydrodynamic simulations of a geometrically thin accretion disk around a non-spinning black hole. The disk has a thickness…

astro-ph2007★ 19 cited

Estimating the Spins of Stellar-Mass Black Holes by Fitting Their Continuum Spectra

Ramesh Narayan, Jeffrey E. McClintock, Rebecca Shafee

We have used the Novikov-Thorne thin disk model to fit the continuum X-ray spectra of three transient black hole X-ray binaries in the thermal state. From the fits we estimate the…

astro-ph2007★ 14 cited

Estimating the Spins of Stellar-Mass Black Holes

Jeffrey E. McClintock, Ramesh Narayan, Rebecca Shafee

We describe a program that we have embarked on to estimate the spins of stellar-mass black holes in X-ray binaries. We fit the continuum X-ray spectrum of the radiation from the ac…

astro-ph2007★ 76 cited

Viscous Torque and Dissipation in the Inner Region of a Thin Accretion Disk: Implications for Measuring Black Hole Spin

Rebecca Shafee, Ramesh Narayan, Jeffrey E. McClintock

We consider a simple Newtonian model of a steady accretion disk around a black hole. The model is based on height-integrated hydrodynamic equations, alpha-viscosity, and a pseudo-N…

astro-ph2006★ 586 cited

The Spin of the Near-Extreme Kerr Black Hole GRS 1915+105

Jeffrey E. McClintock, Rebecca Shafee, Ramesh Narayan +3

Based on a spectral analysis of the X-ray continuum that employs a fully relativistic accretion-disk model, we conclude that the compact primary of the binary X-ray source GRS 1915…