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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.

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Gravity and Light: Combining Gravitational Wave and Electromagnetic Observations in the 2020s

R. J. Foley, +112 more
TL;DR: In this article, the authors outline some of the most exciting scientific questions that can be answered by combining both gravitational wave (GW) and electromagnetic (EM) observations, including new classes of events such as neutron-star-black-hole mergers, corecollapse supernovae, and almost certainly something completely unexpected.
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

Galaxy-Scale Outflows Driven by Active Galactic Nuclei

TL;DR: In this article, the effects of active galactic nuclei (AGN) on interstellar gas in the AGN's host galaxy were studied and theoretical mechanisms that can lead to AGN wind massloading and momentum/energy fluxes large enough to have a significant impact on galaxy formation were discussed.
Journal ArticleDOI

Spherical Accretion with Anisotropic Thermal Conduction

TL;DR: In this paper, the effects of anisotropic thermal conduction on magnetized spherical accretion flows using global axisymmetric MHD simulations were studied. But the authors focused on the effect of the thermal convection on the magnetic field.
Proceedings ArticleDOI

Proto‐Neutron Star Winds, Magnetar Birth, and Gamma‐Ray Bursts

TL;DR: In this article, the mass and energy loss from magnetically driven PNS winds for both relativistic and non-relativistic outflows were derived, including important multi-dimensional considerations.