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astro-ph1999
Is the Plasma Within Bubbles and Superbubbles Hot or Cold?
Mordecai-Mark Mac Low
I review what is known about the temperature of the plasma within stellar wind bubbles and superbubbles. Classical theory suggests that it should be hot, with characteristic temper…
astro-ph1999
MHD Turbulence in Star-Forming Clouds
Mordecai-Mark Mac Low, Ralf Klessen, Fabian Heitsch
We review how supersonic turbulence can both prevent and promote the collapse of molecular clouds into stars. First we show that decaying turbulence cannot significantly delay coll…
astro-ph1999
Characterizing the structure of interstellar turbulence
Mordecai-Mark Mac Low, Volker Ossenkopf
Modeling the structure of molecular clouds depends on good methods to statistically compare simulations with observations in order to constrain the models. Here we characterize a s…