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19962026
most citedOrigin of the heavy elements in binary neutron-star mergers from a gravitational wave event

1.2k citations · 7.7k across the 73 of their papers we have counts for

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16 papers · 1 filter

astro-ph.HE2025

Resolving the (Debate About) Nozzle Shocks in Tidal Disruption Events

Zachary L. Andalman, Eliot Quataert, Eric R. Coughlin +1

When a star passes within the Roche limit of a supermassive black hole (SMBH), it is pulled apart by the BH's tidal field in a tidal disruption event (TDE). The resulting flare is…

astro-ph.HE2025

Estimation of Magnetic Fields from Synchrotron Emission: Numerical Tests

Nora B. Linzer, Lucia Armillotta, Eve C. Ostriker +1

We use models of spectrally resolved cosmic ray (CR) transport in TIGRESS MHD simulations of the local ISM to produce synthetic synchrotron emission and to test, on scales from a f…

astro-ph.HE2025

X-ray Transmission Through Photoionized Gas with Moderate Thomson Optical Depth

Taya Govreen-Segal, Ehud Nakar, Eliot Quataert

We model the absorption of X-rays by gas obscuring the source and photoionized by it. We consider a broad range of column densities, including both Thomson-thin and Thomson-thick m…

astro-ph.GA20251 cited

Second public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation

Andrew Wetzel, Jenna Samuel, Pratik J. Gandhi +34

We describe the second data release (DR2) of the FIRE-2 cosmological zoom-in simulations of galaxy formation, from the Feedback In Realistic Environments (FIRE) project, available…

astro-ph.HE2025

Super-Eddington accretion onto black holes and its application to fallback accretion

Tamar Faran, Eliot Quataert

We study the problem of steady-state spherical accretion onto a black hole, in which the internal energy of the flow is governed by radiation and photon diffusion dominates the ene…

astro-ph.HE2025

Self-Similar Cosmic-Ray Transport in High-Resolution Magnetohydrodynamic Turbulence

Philipp Kempski, Drummond B. Fielding, Eliot Quataert +5

We study the propagation of cosmic rays (CRs) through a simulation of magnetohydrodynamic (MHD) turbulence at unprecedented resolution of . We drive turbulence that is…