activity
20032014
most citedConvective-reactive proton-C12 combustion in Sakurai's object (V4334 Sagittarii) and implications for the evolution and yields from the first generations of stars

231 citations · 1.7k across the 30 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2013★ 7 cited

First Simulations of Core- Collapse Supernovae to Supernova Remnants with SNSPH

Carola I. Ellinger, Gabriel Rockefeller, Christopher L. Fryer +2

We present the first 3-dimensional simulations following the evolution of supernova shocks from their inception in the stellar core through the development of a supernova remnant i…

astro-ph.SR2012★ 130 cited

The 12C + 12C reaction and the impact on nucleosynthesis in massive stars

M. Pignatari, R. Hirschi, M. Wiescher +7

Despite much effort in the past decades, the C-burning reaction rate is uncertain by several orders of magnitude, and the relative strength between the different channels 12C(12C,a…

astro-ph.SR2012★ 48 cited

A Case Study of Small Scale Structure Formation in 3D Supernova Simulations

Carola I. Ellinger, Patrick A. Young, Christopher L. Fryer +1

It is suggested in observations of supernova remnants that a number of large- and small-scale structures form at various points in the explosion. Multidimensional modeling of core-…

astro-ph.SR2011★ 212 cited

Simulating the Common Envelope Phase of a Red Giant Using SPH and Uniform Grid Codes

Jean-Claude Passy, Orsola De Marco, Chris L. Fryer +6

We use three-dimensional hydrodynamical simulations to study the rapid infall phase of the common envelope interaction of a red giant branch star of mass equal to 0.88 \msun and a…

astro-ph.SR2010

The effect of 12C + 12C rate uncertainties on the weak s-process component

Michael E. Bennett, Raphael Hirschi, Marco Pignatari +9

The contribution by massive stars (M > 9 solar masses) to the weak s-process component of the solar system abundances is primarily due to the 22Ne neutron source, which is activate…

astro-ph.SR2010★ 78 cited

56Ni Production in Double Degenerate White Dwarf Collisions

Cody Raskin, Evan Scannapieco, Gabriel Rockefeller +3

We present a comprehensive study of white dwarf collisions as an avenue for creating type Ia supernovae. Using a smooth particle hydrodynamics code with a 13-isotope, α-chain nucle…