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19962009
most citedShort Duration Gamma-Ray Bursts with Extended Emission from Proto-Magnetar Spin-Down

414 citations · 2.6k across the 22 of their papers we have counts for

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Showing 2004 · astro-phShow all

6 papers · 2 filters

astro-ph2004

Synchrotron Radiation From Radiatively Inefficient Accretion Flow Simulations: Applications to Sgr A*

Joshua E. Goldston, Eliot Quataert, Igor V. Igumenshchev

We calculate synchrotron radiation in three-dimensional pseudo-Newtonian magnetohydrodynamic simulations of radiatively inefficient accretion flows. We show that the emission is hi…

astro-ph2004

Core Formation in Galactic Nuclei Due to Recoiling Black Holes

Michael Boylan-Kolchin, Chung-Pei Ma, Eliot Quataert

Anisotropic gravitational radiation from a coalescing black hole binary can impart a recoil velocity of up to several hundred km/s to the remnant black hole. We examine the effects…

astro-ph2004

On the Maximum Luminosity of Galaxies and Their Central Black Holes: Feedback From Momentum-Driven Winds

Norman Murray, Eliot Quataert, Todd A. Thompson

We investigate large-scale galactic winds driven by momentum deposition. Momentum injection is provided by (1) radiation pressure produced by the continuum absorption and scatterin…

astro-ph2004

Viscosity and Rotation in Core-Collapse Supernovae

Todd A. Thompson, Eliot Quataert, Adam Burrows

We construct models of core-collapse supernovae in one spatial dimension, including rotation, angular momentum transport, and viscous dissipation employing an alpha-prescription. W…

astro-ph2004

Testing Radiatively-Inefficient Accretion Flow Theory: an XMM-Newton Observation of NGC 3998

A. Ptak, Y. Terashima, L. C. Ho +1

We present the results of a 10 ks XMM-Newton observation of NGC 3998, a ``type-I'' LINER galaxy. Our goal is to test the extent to which radiatively-inefficient accretion flow (RIA…

astro-ph2004

On The Nature of the Variable Infrared Emission from Sgr A*

Feng Yuan, Eliot Quataert, Ramesh Narayan

Recent infrared (IR) observations of the center of our Galaxy indicate that the supermassive black hole source Sgr A* is strongly variable in the IR. The timescale for the variabil…