activity
19972017
most citedBlack Holes on FIRE: Stellar Feedback Limits Early Feeding of Galactic Nuclei

262 citations · 673 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2017★ 262 cited

Black Holes on FIRE: Stellar Feedback Limits Early Feeding of Galactic Nuclei

Daniel Anglés-Alcázar, Claude-André Faucher-Giguère, Eliot Quataert +5

We introduce massive black holes (BHs) in the Feedback In Realistic Environments project and perform high-resolution cosmological hydrodynamic simulations of quasar-mass halos ($M_…

astro-ph2008★ 121 cited

X-ray observations of the galaxy cluster PKS 0745-191: To the virial radius, and beyond

Matthew R. George, Andrew C. Fabian, Jeremy S. Sanders +2

We measure X-ray emission from the outskirts of the cluster of galaxies PKS 0745-191 with Suzaku, determining radial profiles of density, temperature, entropy, gas fraction, and ma…

astro-ph2007★ 7 cited

Star Formation at Zero and Very Low Metallicities

Jonathan C. Tan, Christopher F. McKee

We describe how star formation is expected to proceed in the early metal-free Universe, focusing on the very first generations of stars. We then discuss how the star formation proc…

astro-ph2007

Magnetar Driven Bubbles and the Origin of Collimated Outflows from GRBs

N. Bucciantini, E. Quataert, J. Arons +2

We model the interaction between the wind from a newly formed rapidly rotating magnetar and the surrounding progenitor. In the first few seconds after core collapse the magnetar in…

astro-ph2007★ 139 cited

Relativistic Jets and Long-Duration Gamma-ray Bursts from the Birth of Magnetars

N. Bucciantini, E. Quataert, J. Arons +2

We present time-dependent axisymmetric magnetohydrodynamic simulations of the interaction of a relativistic magnetized wind produced by a proto-magnetar with a surrounding stellar…

astro-ph2007★ 111 cited

Magnetar Driven Bubbles and the Origin of Collimated Outflows in Gamma-ray Bursts

N. Bucciantini, E. Quataert, J. Arons +2

We model the interaction between the wind from a newly formed rapidly rotating magnetar and the surrounding supernova shock and host star. The dynamics is modeled using the two-dim…