29 citations · 29 across the 2 of their papers we have counts for
8 papers
Parameters of the Supernova-Driven Interstellar Turbulence
Luke Chamandy, Anvar Shukurov
Galactic dynamo models take as input certain parameters of the interstellar turbulence, most essentially the correlation time , root-mean-square turbulent speed , and correla…
Common Envelope Evolution on the Asymptotic Giant Branch: Unbinding within a Decade?
Luke Chamandy, Eric G. Blackman, Adam Frank +2
Common envelope (CE) evolution is a critical but still poorly understood progenitor phase of many high-energy astrophysical phenomena. Although 3D global hydrodynamic CE simulation…
Synthesizing Observations and Theory to Understand Galactic Magnetic Fields: Progress and Challenges
Rainer Beck, Luke Chamandy, Ed Elson +1
Constraining dynamo theories of magnetic field origin by observation is indispensable but challenging, in part because the basic quantities measured by observers and predicted by m…
Bipolar Planetary Nebulae from Outflow Collimation by Common Envelope Evolution
Yangyuxin Zou, Adam Frank, Zhuo Chen +8
The morphology of bipolar planetary nebulae (PNe) can be attributed to interactions between a fast wind from the central engine and dense toroidal shaped ejecta left over from comm…
The impact of recombination energy on simulations of the common envelope binary interaction
Thomas Reichardt, Orsola De Marco, Roberto Iaconi +1
During the common envelope binary interaction, the expanding layers of the gaseous common envelope recombine and the resulting recombination energy has been suggested as a contribu…
How Drag Force Evolves in Global Common Envelope Simulations
Luke Chamandy, Eric G. Blackman, Adam Frank +3
We compute the forces, torque and rate of work on the companion-core binary due to drag in global simulations of common envelope (CE) evolution for three different companion masses…