activity
19972011
most citedThermonuclear (type-I) X-ray bursts observed by the Rossi X-ray Timing Explorer

751 citations · 1.8k across the 19 of their papers we have counts for

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Showing 2006Show all

6 papers · 1 filter

astro-ph20065 cited

Spectral Methods for Time-Dependent Studies of Accretion Flows. III. Three-Dimensional, Self-gravitating, Magnetohydrodynamic Disks

Chi-kwan Chan, Dimitrios Psaltis, Feryal Ozel

Accretion disks are three-dimensional, turbulent, often self-gravitating, magnetohydrodynamic flows, which can be modeled in detail with numerical simulations. In this paper, we pr…

astro-ph200629 cited

Constraints on Braneworld Gravity Models from a Kinematic Limit on the Age of the Black Hole XTE J1118+480

Dimitrios Psaltis

In braneworld gravity models with a finite AdS curvature in the extra dimension, the AdS/CFT correspondence leads to a prediction for the lifetime of astrophysical black holes that…

astro-ph200647 cited

The fundamental difference between shear alpha viscosity and turbulent magnetorotational stresses

Martin E. Pessah, Chi-kwan Chan, Dimitrios Psaltis

Numerical simulations of turbulent, magnetized, differentially rotating flows driven by the magnetorotational instability are often used to calculate the effective values of alpha…

astro-ph200656 cited

A Local Model for Angular Momentum Transport in Accretion Disks Driven by the Magnetorotational Instability

Martin E. Pessah, Chi-kwan Chan, Dimitrios Psaltis

We develop a local model for the exponential growth and saturation of the Reynolds and Maxwell stresses in turbulent flows driven by the magnetorotational instability. We first der…

astro-ph2006751 cited

Thermonuclear (type-I) X-ray bursts observed by the Rossi X-ray Timing Explorer

Duncan K. Galloway, Michael P. Muno, Jacob M. Hartman +2

We have assembled a sample of 1187 thermonuclear (type-I) X-ray bursts from 48 accreting neutron stars by the Rossi X-ray Timing Explorer, spanning more than ten years. The sample…

astro-ph200671 cited

The signature of the magnetorotational instability in the Reynolds and Maxwell stress tensors in accretion discs

Martin E. Pessah, Chi-kwan Chan, Dimitrios Psaltis

The magnetorotational instability is thought to be responsible for the generation of magnetohydrodynamic turbulence that leads to enhanced outward angular momentum transport in acc…