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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

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astro-ph2008★ 17 cited

Howes et al. Reply

G. G. Howes, S. C. Cowley, W. Dorland +4

Howes et al. Reply to Comment on "Kinetic Simulations of Magnetized Turbulence in Astrophysical Plasmas" arXiv:0711.4355

astro-ph2008★ 84 cited

Nickel-Rich Outflows from Accretion Disks Formed by the Accretion-Induced Collapse of White Dwarfs

B. D. Metzger, A. L. Piro, E. Quataert

A white dwarf (WD) approaching the Chandrasekhar mass may in several cases undergo accretion-induced collapse (AIC) to a neutron star (NS) before a thermonuclear explosion ensues.…

astro-ph2008★ 205 cited

GRB 080503: Implications of a Naked Short Gamma-Ray Burst Dominated by Extended Emission

D. A. Perley, B. D. Metzger, J. Granot +22

We report on observations of GRB 080503, a short gamma-ray burst with very bright extended emission (about 30 times the gamma-ray fluence of the initial spike) in conjunction with…

astro-ph2008★ 110 cited

Neutron-Rich Freeze-Out in Viscously Spreading Accretion Disks Formed from Compact Object Mergers

B. D. Metzger, A. L. Piro, E. Quataert

Accretion disks with masses ~0.001-0.1 Msun form during the merger of neutron star (NS)-NS and black hole-NS binaries. Initially, such hyper-accreting disks cool efficiently by neu…

astro-ph2008★ 216 cited

Time-Dependent Models of Accretion Disks Formed from Compact Object Mergers

B. D. Metzger, A. L. Piro, E. Quataert

We present time-dependent models of the accretion disks created during compact object mergers, focusing on the energy available from accretion at late times and the composition of…

astro-ph2008★ 49 cited

Spherical Accretion with Anisotropic Thermal Conduction

Prateek Sharma, Eliot Quataert, James M. Stone

We study the effects of anisotropic thermal conduction on magnetized spherical accretion flows using global axisymmetric MHD simulations. In low collisionality plasmas, the Bondi s…