E
Eliot Quataert
Researcher at University of California, Berkeley
Publications - 242
Citations - 15951
Eliot Quataert is an academic researcher from University of California, Berkeley. The author has contributed to research in topics: Galaxy & Accretion (astrophysics). The author has an hindex of 66, co-authored 242 publications receiving 14271 citations. Previous affiliations of Eliot Quataert include University of California & UCB.
Papers
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Journal ArticleDOI
Exploring the epoch of hydrogen reionization using FRBs
TL;DR: In this article, the authors describe three different methods for exploring the hydrogen reionization epoch using fast radio bursts (FRBs) and provide arguments for the existence of FRBs at high redshift (z).
Journal ArticleDOI
Magnetic Fields in Starburst Galaxies and The Origin of the FIR-Radio Correlation
TL;DR: In this paper, the authors assess a number of independent constraints on the magnetic field strength in starbursts and conclude that magnetic fields in starburst galaxies are significantly larger than B_min.
Book ChapterDOI
Astrophysical Evidence for Black Hole Event Horizons
TL;DR: In binary star systems, consisting of two stars revolving around each other under the influence of their mutual gravitational attraction, black holes with masses of order several solar masses (M ~ 5 − 20M⊙) are thought to exist as the dead remnant of the initially more massive of the two stars as discussed by the authors.
Journal ArticleDOI
The Impact of Type Ia Supernovae in Quiescent Galaxies. II. Energetics and Turbulence
TL;DR: In this article, a series of high-resolution simulations to examine the energetics and turbulence of the medium under SNe Ia supernovae are presented. But their effects differ distinctly from a volumetric heating term, as is commonly assumed in unresolved simulations.
Journal ArticleDOI
The Structure of Radiatively Inefficient Black Hole Accretion Flows
TL;DR: In this article, the authors run three long-timescale general-relativistic magnetohydrodynamic simulations of radiatively inefficient accretion flows onto non-rotating black holes and understand the resulting flow structure.