activity
19972004
most citedGravoturbulent Star Cluster Formation

3 citations · 3 across the 3 of their papers we have counts for

collaborators

16 papers

astro-ph2004

Magnetized Turbulence

Mordecai-Mark Mac Low

Several topics in the theory of magnetized turbulence are reviewed with application to star formation and the interstellar medium. The density, pressure, and temperature distributi…

astro-ph20043 cited

Gravoturbulent Star Cluster Formation

Ralf S. Klessen, Javier Ballesteros-Paredes, Yuexing Li +1

Stars form by gravoturbulent fragmentation of interstellar gas clouds. The supersonic turbulence ubiquitously observed in Galactic molecular gas generates strong density fluctuatio…

astro-ph2002

Turbulence in the Interstellar Medium: Energetics and Driving Mechanisms

Mordecai-Mark Mac Low

Interstellar turbulence is expected to dissipate quickly in the absence of continuous energy input. I examine the energy available for driving the turbulence from six likely mechan…

astro-ph2002

MHD Turbulence in Star-Forming Regions and the Interstellar Medium

Mordecai-Mark Mac Low

MHD turbulence plays a central role in the physics of star-forming molecular clouds and the interstellar medium. I here show that MHD turbulence in molecular clouds must be driven…

astro-ph2001

Mixing of Primordial Elements in a Supernova-Driven ISM

Miguel A. de Avillez, Mordecai-Mark Mac Low

In order to understand the time scales for complete mixing in a supernova-driven ISM we used the model of Avillez (2000) to follow the mixing and dispersal of inhomogeneities with…

astro-ph2001

Column Density Probability Distribution Functions in Turbulent Molecular Clouds: A Comparison between Theory and Observations

Andreas Burkert, Mordecai-Mark Mac Low

The one-point statistics of column density distributions of turbulent molecular cloud models are investigated and compared with observations. In agreement with the observations, th…