activity
19962025
most citedSimulating the Common Envelope Phase of a Red Giant Using SPH and Uniform Grid Codes

212 citations · 390 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2025★ 1 cited

Aeos is Mixing it Up: The (In)homogeneity of Metal Mixing Following Population III Star Formation

Jennifer Mead, Kaley Brauer, Greg L. Bryan +7

Stellar surface abundances are records of the state of the gas from which stars formed, and thus trace how individual elements have mixed into the surrounding medium following thei…

astro-ph.GA2024

Massive Star Cluster Formation with Binaries. I. Evolution of Binary Populations

Claude Cournoyer-Cloutier, Alison Sills, William E. Harris +7

We study the evolution of populations of binary stars within massive cluster-forming regions. We simulate the formation of young massive star clusters within giant molecular clouds…

astro-ph.EP2018★ 96 cited

Diffusion and Concentration of Solids in the Dead Zone of a Protoplanetary Disk

Chao-Chin Yang, Mordecai-Mark Mac Low, Anders Johansen

The streaming instability is a promising mechanism to drive the formation of planetesimals in protoplanetary disks. To trigger this process, it has been argued that sedimentation o…

astro-ph.GA2018★ 35 cited

Effect of the heating rate on the stability of the three-phase interstellar medium

Alex S. Hill, Mordecai-Mark Mac Low, Andrea Gatto +1

We investigate the impact of the far ultraviolet (FUV) heating rate on the stability of the three-phase interstellar medium using three-dimensional simulations of a kpc, ve…

astro-ph.EP2018★ 4 cited

Dust concentration and chondrule formation

Alexander Hubbard, Mordecai-Mark Mac Low, Denton S. Ebel

Meteoritical and astrophysical models of planet formation make contradictory predictions for dust concentration factors in chondrule forming regions of the solar nebula. Meteoritic…

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…