3 citations · 3 across the 3 of their papers we have counts for
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astro-ph1997
Structure and Dynamics of Magnetized Interstellar Clouds: Super-Alfvenic Turbulence?
Mordecai-Mark Mac Low
This review summarizes the argument for molecular clouds being dominated by turbulence, most likely super-Alfvenic turbulence. Five lines of observational evidence are given: molec…
astro-ph1997
The formation of C-shocks: structure and signatures
Michael D. Smith, Mordecai-Mark Mac Low
Shock waves in molecular clouds should evolve into continuous or C-type structures due to the magnetic field and ion-neutral friction. We here determine whether and how this is ach…