237 citations · 1.4k across the 50 of their papers we have counts for
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Energy Budget and Core-Envelope Motion in Common Envelope Evolution
Luke Chamandy, Yisheng Tu, Eric G. Blackman +4
We analyze a 3D hydrodynamic simulation of common envelope evolution to understand how energy is transferred between various forms and whether theory and simulation are mutually co…
Calculating turbulent transport tensors by averaging single plume dynamics and application to dynamos
Hongzhe Zhou, Eric G. Blackman
Transport coefficients in turbulence are comprised of correlation functions between turbulent fluctuations and efficient methods to calculate them are desirable. For example, in me…
Photoevaporative Flows From Exoplanet Atmospheres: A 3-D Radiative Hydrodynamic Parameter Study
Alex Debrecht, Jonathan Carroll-Nellenback, Adam Frank +3
The photoionization-driven evaporation of planetary atmospheres has emerged as a potentially fundamental process for planets on short period orbits. While 1-D studies have proven t…
Accretion in Common Envelope Evolution
Luke Chamandy, Adam Frank, Eric G. Blackman +6
Common envelope evolution (CEE) occurs in some binary systems involving asymptotic giant branch (AGB) or red giant branch (RGB) stars, and understanding this process is crucial for…
Planetary Nebulae Shaped By Common Envelope Evolution
Adam Frank, Zhuo Chen, Thomas Reichardt +3
The morphologies of planetary nebula have long been believed to be due to wind shaping processes in which a fast wind from the central star impacts a previously ejected envelope. A…
Accretion in common envelope evolution
Luke Chamandy, Adam Frank, Eric G. Blackman +6
Common envelope evolution (CEE) is presently a poorly understood, yet critical, process in binary stellar evolution. Characterizing the full 3D dynamics of CEE is difficult in part…