3 citations · 3 across the 3 of their papers we have counts for
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Clustered vs. Isolated Star Formation
Mordecai-Mark Mac Low
I argue that star formation is controlled by supersonic turbulence, drawing for support on a number of 3D hydrodynamical and MHD simulations as well as theoretical arguments. Clust…
The distribution of shock waves in driven supersonic turbulence
Michael D. Smith, Mordecai-Mark Mac Low, Fabian Heitsch
Supersonic turbulence generates distributions of shock waves. Here, we analyse the shock waves in three-dimensional numerical simulations of uniformly driven supersonic turbulence,…
The Dynamical Interstellar Medium: Insights from Numerical Models
Mordecai-Mark Mac Low
Numerical models of the dynamical interstellar medium show that interactions between structures such as supernova remnants and superbubbles are more important than the structures t…
The shock waves in decaying supersonic turbulence
Michael D. Smith, Mordecai-Mark Mac Low, Julia M. Zuev
We here analyse numerical simulations of supersonic, hypersonic and magnetohydrodynamic turbulence that is free to decay. Our goals are to understand the dynamics of the decay and…