151 citations · 490 across the 28 of their papers we have counts for
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astro-ph.GA2026
From IFS Maps to 3D Structure I: Constraining Geometry in the Circumgalactic Medium
Mandy C. Chen, Michael Rauch, Zhijie Qu +3
The three-dimensional geometric structure of the cool (T~ K) circumgalactic medium (CGM) -- the line-of-sight depth and the number of discrete clumps -- is poorly constrained…
physics.plasm-ph2026
Numerical simulations of shock-driven, supersonic interstellar turbulence in colliding three-temperature laboratory plasmas
Stefano Merlini, James R. Beattie, Vicente Valenzuela-Villaseca
Shock-driven turbulence is central to astrophysical plasmas in which explosions and compressive driving inject energy through shocks rather than steady stirring. We present three-d…
astro-ph.GA2026
What is the Strouhal number of turbulence driven by supernovae?
James R. Beattie, Isabelle Connor, Enrico Ramirez-Ruiz
The Strouhal number, , measures the temporal coherence of turbulent driving relative to the outer-scale eddy turnover time. In turbulence-box mod…