activity
19972023
most citedHow Massive Single Stars End their Life

2.2k citations · 21.5k across the 170 of their papers we have counts for

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Showing 2011Show all

5 papers · 1 filter

astro-ph.HE2011★ 3 cited

Conservative Initial Mapping For Multidimensional Simulations of Stellar Explosions

Ke-Jung Chen, Alexander Heger, Ann Almgren

Mapping one-dimensional stellar profiles onto multidimensional grids as initial conditions for hydrodynamics calculations can lead to numerical artifacts, one of the most severe of…

astro-ph.HE2011★ 157 cited

Long Gamma-Ray Transients from Collapsars

S. E. Woosley, Alexander heger

In the collapsar model for common gamma-ray bursts, the formation of a centrifugally supported disk occurs during the first 10 seconds following the collapse of the iron core…

astro-ph.HE2011★ 51 cited

Multi-Zone Models of Superbursts from Accreting Neutron Stars

L. Keek, A. Heger

Superbursts are rare and energetic thermonuclear carbon flashes observed to occur on accreting neutron stars. We create the first multi-zone models of series of superbursts using a…

astro-ph.HE2011

Multidimensional Simulations of Thermonuclear Supernovae from the First Stars

Ke-Jung Chen, Alexander Heger, Ann Almgren

Theoretical models suggest that the first stars in the universe could have been very massive, with typical masses 100 \Msun. Many of them might have died as energetic the…

astro-ph.HE2011★ 261 cited

Pair Instability Supernovae: Light Curves, Spectra, and Shock Breakout

Daniel Kasen, S. E. Woosley, Alexander Heger

For the initial mass range (140 < M < 260 Msun) stars die in a thermonuclear runaway triggered by the pair-production instability. The supernovae they make can be remarkably energe…