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19972022
most citedLow-Mass Binary Induced Outflows from Asymptotic Giant Branch Stars

237 citations · 1.4k across the 50 of their papers we have counts for

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Showing 2018Show all

7 papers · 1 filter

astro-ph.SR2018

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…

astro-ph.SR2018

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…

astro-ph.EP2018

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…

astro-ph.SR2018

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…

astro-ph.SR2018

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…

astro-ph.SR2018

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…