activity
19952026
most citedGalaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation

1.5k citations · 52.3k across the 433 of their papers we have counts for

collaborators
Showing 2013Show all

10 papers · 1 filter

astro-ph.SR2013★ 41 cited

Dynamical resonance locking in tidally interacting binary systems

Joshua Burkart, Eliot Quataert, Phil Arras

We examine the dynamics of resonance locking in detached, tidally interacting binary systems. In a resonance lock, a given stellar or planetary mode is trapped in a highly resonant…

astro-ph.CO2013★ 1.5k cited

Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation

Philip F. Hopkins, Dusan Keres, Jose Onorbe +4

We present a series of high-resolution cosmological simulations of galaxy formation to z=0, spanning halo masses ~10^8-10^13 M_sun, and stellar masses ~10^4-10^11. Our simulations…

astro-ph.GA2013★ 21 cited

The Role of Magnetic Fields in Starburst Galaxies as Revealed by OH Megamasers

James McBride, Eliot Quataert, Carl Heiles +1

We present estimates of magnetic field strengths in the interstellar media of starburst galaxies derived from measurements of Zeeman splitting associated with OH megamasers. The re…

astro-ph.GA2013★ 45 cited

Hot Galactic Winds Constrained by the X-Ray Luminosities of Galaxies

Dong Zhang, Todd A. Thompson, Norman Murray +1

Galactic superwinds may be driven by very hot outflows generated by overlapping supernovae within the host galaxy. We use the Chevalier & Clegg (CC85) wind model and the observed c…

astro-ph.SR2013★ 39 cited

Perpendicular Ion Heating by Reduced Magnetohydrodynamic Turbulence

Qian Xia, Jean C. Perez, Benjamin D. G. Chandran +1

Recent theoretical studies argue that the rate of stochastic ion heating in low-frequency Alfvén-wave turbulence is given by , where is…

astro-ph.SR2013★ 220 cited

Setting the Stage for Circumstellar Interaction in Core-Collapse Supernovae II: Wave-Driven Mass Loss in Supernova Progenitors

Joshua H. Shiode, Eliot Quataert

Supernovae (SNe) powered by interaction with circumstellar material provide evidence for intense stellar mass loss during the final years leading up to core collapse. We have argue…